
corpus = """

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The universe is incredibly vast and constantly expanding.
Did you know that the Milky Way galaxy contains over 100 billion stars?
Black holes are regions of space where gravity is so strong that not even light can escape.
The Hubble Space Telescope has provided us with breathtaking images of distant galaxies.
The closest star to Earth, other than the Sun, is Proxima Centauri.
Space exploration has led to significant technological advancements and discoveries.
The speed of light is approximately 299,792 kilometers per second.
The International Space Station orbits Earth at an average altitude of around 400 kilometers.
Astronomers use radio telescopes to observe celestial objects that emit radio waves.
Jupiter is the largest planet in our solar system, with a diameter of about 139,820 kilometers.
The concept of a black hole was first proposed by physicist John Michell in 1783.
The observable universe is estimated to be about 93 billion light-years in diameter.
Saturn’s rings are made up of ice, dust, and rocky particles.
The Andromeda Galaxy is the nearest spiral galaxy to the Milky Way.
Cosmic microwave background radiation is the afterglow of the Big Bang.
Apple Inc. is known for its innovative technology products and software.
The latest iPhone models feature advanced camera systems and powerful processors.
macOS is Apple's operating system for Mac computers, known for its sleek design and functionality.
Apple's ecosystem includes devices like the iPad, Apple Watch, and Apple TV.
The App Store offers a wide range of applications for iOS devices.
Apple's M1 chip represents a significant leap in performance and efficiency for Mac computers.
The Apple Watch includes health and fitness features such as heart rate monitoring and GPS tracking.
Tim Cook is the CEO of Apple Inc., succeeding Steve Jobs.
Apple's iCloud service provides cloud storage and synchronization across devices.
The iPad Pro features a high-resolution display and compatibility with the Apple Pencil.
Apple introduced the first iPhone in 2007, revolutionizing the smartphone industry.
The company's headquarters is located in Cupertino, California, known as Apple Park.
Apple's retail stores are designed to provide a unique customer experience with hands-on product demonstrations.
The AirPods offer wireless audio and seamless integration with Apple devices.
Apple’s iOS operating system powers the iPhone, iPad, and iPod Touch.
Science is a systematic enterprise that builds and organizes knowledge in the form of testable explanations and predictions.
The scientific method involves making observations, forming a hypothesis, conducting experiments, and analyzing data.
Photosynthesis is the process by which green plants convert sunlight into chemical energy.
Newton's laws of motion describe the relationship between a body and the forces acting on it.
DNA (deoxyribonucleic acid) carries genetic information in living organisms.
The theory of evolution explains the diversity of life through natural selection.
The periodic table organizes chemical elements based on their atomic number and properties.
Quantum mechanics explores the behavior of particles at the atomic and subatomic levels.
The theory of relativity, proposed by Albert Einstein, describes the relationship between space and time.
Plate tectonics is the theory that Earth's outer shell is divided into several plates that glide over the mantle.
Vaccines are biological preparations that provide immunity against specific diseases.
The laws of thermodynamics govern the principles of energy transfer and conversion.
The study of ecosystems and their interactions is known as ecology.
Gravitational waves are ripples in spacetime caused by massive accelerating objects.
Mathematics is the study of numbers, shapes, and patterns, and their relationships and properties.
Algebra involves solving equations and understanding relationships between variables.
Calculus is the study of change and motion, involving derivatives and integrals.
Geometry focuses on the properties and relations of points, lines, surfaces, and solids.
Statistics involves the collection, analysis, interpretation, and presentation of data.
The Pythagorean theorem states that in a right-angled triangle, the square of the hypotenuse is equal to the sum of the squares of the other two sides.
Trigonometry studies the relationships between the angles and sides of triangles.
Linear algebra deals with vector spaces and linear mappings between these spaces.
The Fibonacci sequence is a series of numbers where each number is the sum of the two preceding ones.
Probability measures the likelihood of a specific event occurring.
Complex numbers include a real part and an imaginary part and are used in various fields of mathematics.
Differential equations involve functions and their derivatives and are used to model real-world phenomena.
Calculus concepts like limits, continuity, and derivatives are fundamental to advanced mathematical analysis.
Number theory explores the properties and relationships of integers.
Mathematics plays a crucial role in fields such as engineering, physics, economics, and computer science.
The Milky Way is just one of billions of galaxies in the universe.
Our solar system is located in the Orion Arm of the Milky Way galaxy.
The Sun is a medium-sized star with a surface temperature of about 5,500 degrees Celsius.
Neutron stars are incredibly dense remnants of supernova explosions.
The concept of space-time combines the three dimensions of space with the dimension of time.
A supernova is the explosion of a star at the end of its lifecycle.
NASA's Mars rovers have provided invaluable data about the Red Planet's surface.
Astronomers use spectroscopy to analyze the light emitted by stars and galaxies.
The Hubble Space Telescope has captured some of the most detailed images of distant galaxies.
Saturn's largest moon, Titan, has a thick atmosphere and is known for its methane lakes.
Black holes can be detected by observing the effects of their gravity on nearby objects.
The Voyager probes have traveled beyond our solar system and continue to send data back to Earth.
Jupiter's Great Red Spot is a massive storm that has been raging for centuries.
The concept of dark matter refers to the invisible substance that makes up a significant portion of the universe's mass.
The Andromeda Galaxy is on a collision course with the Milky Way, predicted to merge in about 4.5 billion years.
Cosmic rays are high-energy particles from space that continuously bombard Earth.
A quasar is an extremely luminous active galactic nucleus powered by a supermassive black hole.
The expansion of the universe was first observed by Edwin Hubble in the 1920s.
Astronauts experience microgravity, which affects their bodies in various ways during space travel.
The discovery of exoplanets has expanded our understanding of potential habitable worlds beyond our solar system.
The Kuiper Belt is a region of the solar system beyond Neptune that contains many small icy bodies.
The James Webb Space Telescope aims to explore the early universe and study distant galaxies.
Neutrinos are elusive subatomic particles that pass through matter almost undetected.
The event horizon of a black hole is the boundary beyond which nothing can escape.
The concept of a multiverse suggests that our universe may be just one of many.
Dark energy is thought to be responsible for the accelerated expansion of the universe.
The lunar surface is covered in a layer of fine dust called regolith.
The International Space Station is a joint project involving multiple space agencies from around the world.
The Solar System's asteroid belt lies between the orbits of Mars and Jupiter.
Gamma-ray bursts are the most energetic explosions observed in the universe.
Solar flares are sudden eruptions of intense radiation from the Sun's surface.
Space weather can impact satellite operations and communications on Earth.
The Moon's gravitational influence causes ocean tides on Earth.
Astronomers use radio waves to study celestial objects that emit at these frequencies.
The concept of spacetime curvature is central to Einstein's theory of General Relativity.
The observable universe is estimated to be about 13.8 billion years old.
A light-year is a measure of distance, equal to the distance light travels in one year.
The Roche limit is the distance within which a celestial body, held together by gravity, will be torn apart by tidal forces.
The Cassini spacecraft provided detailed information about Saturn and its rings before its mission ended.
Astrobiology is the study of the origin, evolution, and possibility of life elsewhere in the universe.
Pulsars are rotating neutron stars that emit beams of radiation.
The cosmic microwave background radiation is a remnant of the Big Bang.
The term "exoplanet" refers to planets located outside our solar system.
The LIGO observatory has detected gravitational waves from colliding black holes.
The Drake Equation estimates the number of active, communicative extraterrestrial civilizations in our galaxy.
Magnetars are a type of neutron star with an extremely strong magnetic field.
The Voyager 1 spacecraft is the farthest human-made object from Earth.
Comets are icy bodies that release gas and dust, forming a glowing coma and tail when close to the Sun.
The Great Attractor is a mysterious gravitational anomaly affecting the motion of galaxies.
The Big Bang Theory is the leading explanation for the origin of the universe.
The solar wind is a stream of charged particles released from the Sun's outer layers.
Elliptical galaxies have a smooth, featureless light distribution and lack the distinct arms of spiral galaxies.
The concept of cosmic inflation proposes that the universe expanded rapidly in its early moments.
The Nebula is a cloud of gas and dust in space, often serving as a stellar nursery.
Astronomical units are used to measure distances within our solar system, with one AU equal to the average distance between Earth and the Sun.
Redshift occurs when light from an object is stretched to longer wavelengths as it moves away from us.
The theory of general relativity revolutionized our understanding of gravity and space-time.
The Sun's core is where nuclear fusion occurs, producing the energy that powers the Sun.
Solar eclipses occur when the Moon passes between Earth and the Sun, casting a shadow on Earth.
The distance between Earth and the Sun is approximately 93 million miles or 150 million kilometers.
Space probes are unmanned spacecraft designed to collect data about celestial objects.
A white dwarf is a dense, cooling remnant of a star that has exhausted its nuclear fuel.
The Milky Way's central bulge contains a supermassive black hole known as Sagittarius A*.
Astronomers use the term "light-year" to describe vast distances in space.
The event horizon of a black hole is the boundary where escape velocity exceeds the speed of light.
The solar system's largest planet, Jupiter, has a strong magnetic field and numerous moons.
Astronomical observations have revealed that the universe is expanding at an accelerating rate.
The concept of a wormhole involves a hypothetical tunnel-like structure connecting distant regions of space-time.
Meteor showers occur when Earth passes through the debris left by a comet.
A red giant is a later stage in a star's lifecycle characterized by an expanded, cooler outer envelope.
Spacecraft that land on celestial bodies often use landing gear to absorb the impact.
The Kuiper Belt contains many small, icy objects and is home to dwarf planets like Pluto.
The concept of dark energy is used to explain the observed acceleration of the universe's expansion.
Neutron stars are incredibly compact, with masses greater than the Sun compressed into a sphere about 20 kilometers across.
The term "event horizon" refers to the boundary beyond which nothing can escape a black hole's gravitational pull.
Galaxies are massive systems of stars, gas, dust, and dark matter bound together by gravity.
The study of cosmic microwave background radiation helps scientists understand the early universe.
A pulsar's regular pulses of radiation are caused by its rapid rotation and strong magnetic field.
The search for extraterrestrial intelligence involves monitoring signals from space for potential signs of alien life.
Astronomers use the Doppler effect to measure the movement and velocity of celestial objects.
The concept of time dilation in relativity suggests that time moves slower in stronger gravitational fields.
A supernova can outshine an entire galaxy for a brief period and is a key event in stellar evolution.
Space missions often involve complex calculations to ensure successful trajectories and landing.
Cosmology is the scientific study of the large-scale properties and evolution of the universe.
The Oort Cloud is a spherical shell of icy objects surrounding the solar system at a great distance.
The temperature of space varies widely depending on location and proximity to stars.
Astronomers use gravitational lensing to study distant objects by observing how their light is bent around massive objects.
The concept of a habitable zone refers to the region around a star where conditions may be suitable for life.
The Sun's outer atmosphere, known as the corona, is visible during a total solar eclipse.
Astronomical observations are often conducted using ground-based and space-based telescopes.
Cosmic background radiation provides a snapshot of the universe when it was just 380,000 years old.
A neutron star's intense gravity can cause it to collapse further into a black hole if it accumulates enough mass.
The term "quasar" refers to a very energetic and distant active galactic nucleus.
Astronomers use parallax to measure the distances to nearby stars.
The concept of entropy describes the degree of disorder or randomness in a system.
The discovery of exoplanets has expanded our understanding of planetary systems beyond our own.
A supernova can trigger the formation of new stars by compressing surrounding gas and dust.
The solar system's asteroid belt contains thousands of small rocky bodies orbiting the Sun.
The term "zodiacal light" refers to a faint, diffuse glow seen in the night sky caused by sunlight scattering off interplanetary dust.
The concept of the observable universe is limited by the distance light has traveled since the Big Bang.
Gamma-ray bursts are the most energetic explosions observed in the universe, often associated with the collapse of massive stars.
The study of stellar spectra allows astronomers to determine the composition, temperature, and velocity of stars.
The Hubble Space Telescope has provided detailed images of distant galaxies, nebulae, and other celestial phenomena.
The Solar System's outermost region, known as the heliopause, marks the boundary where the solar wind slows down and merges with the interstellar medium.
The term "black hole" refers to a region of space where gravitational forces are so strong that nothing, not even light, can escape.
Astronomers use redshift to measure the rate at which galaxies are moving away from us, providing evidence for the expanding universe.
The concept of dark matter helps explain the observed gravitational effects on visible matter in galaxies and galaxy clusters.
Space missions like the Apollo program have provided valuable data about the Moon and its surface.
The study of cosmic rays helps scientists understand high-energy processes occurring in space.
Astronomers use the term "cosmic microwave background" to describe the faint radiation left over from the Big Bang.
The theory of relativity, developed by Albert Einstein, revolutionized our understanding of space, time, and gravity.
The concept of a wormhole involves a hypothetical tunnel connecting distant regions of space-time, potentially allowing faster-than-light travel.
Neutrinos are elementary particles that interact very weakly with matter and can pass through entire planets.
Astronomers use space probes to explore the outer reaches of the solar system and beyond.
The concept of a multiverse suggests that our universe may be one of many universes with varying properties.
The study of the interstellar medium helps scientists understand the composition and behavior of matter between stars.
The Sun's energy is produced through nuclear fusion reactions occurring in its core.
The term "light-year" is used to describe the distance that light travels in one year, approximately 5.88 trillion miles or 9.46 trillion kilometers.
A galaxy's central black hole can influence the motion and distribution of stars within the galaxy.
The concept of dark energy is used to explain the observed acceleration of the universe's expansion.
Cosmic inflation proposes that the universe underwent a rapid expansion in its early moments, leading to its current large scale.
Astronomers use the term "Hubble's Law" to describe the relationship between a galaxy's distance and its recessional velocity.
The study of planetary atmospheres helps scientists understand the conditions that may support life on other planets.
The concept of space-time curvature explains how massive objects like stars and planets warp the fabric of space-time.
A supernova remnant is the leftover material from a star's explosion and can lead to the formation of new stars and planetary systems.
The Oort Cloud is a theoretical region of icy bodies surrounding the solar system at a great distance, thought to be the source of long-period comets.
The study of cosmic background radiation provides insight into the early universe and the conditions present shortly after the Big Bang.
The term "event horizon" refers to the boundary around a black hole beyond which nothing can escape its gravitational pull.
The concept of gravitational waves involves ripples in space-time caused by accelerating masses, such as merging black holes or neutron stars.
Astronomers use the term "distant galaxies" to refer to galaxies that are billions of light-years away, providing information about the early universe.
The study of the cosmic microwave background helps scientists understand the universe's origins and evolution.
The term "cosmic rays" refers to high-energy particles from space that can have significant effects on Earth's atmosphere and technology.
Astronomers use the Doppler effect to measure the velocity of celestial objects based on the shift in the wavelength of their emitted light.
The study of interstellar dust and gas provides insights into the processes of star formation and the composition of the universe.
The concept of a black hole's "singularity" refers to a point of infinite density at the center where gravitational forces are extremely strong.
The study of exoplanets involves identifying and characterizing planets orbiting stars outside our solar system.
The concept of "time dilation" explains how time passes more slowly in stronger gravitational fields or at higher velocities.
Astronomers use the term "nebula" to describe a cloud of gas and dust in space where new stars and planetary systems can form.
The study of cosmic microwave background radiation provides a snapshot of the universe when it was just 380,000 years old.
A pulsar is a highly magnetized, rotating neutron star that emits beams of radiation from its magnetic poles.
The term "cosmic inflation" refers to the rapid expansion of the universe in its early moments, leading to its current large scale.
The concept of "spacetime" combines the three dimensions of space with the dimension of time into a unified framework.
Astronomers use the term "gravitational lensing" to describe the bending of light around massive objects, such as galaxy clusters.
The study of dark matter helps explain the discrepancies between the observed and expected distributions of mass in the universe.
The concept of "quasars" involves extremely luminous active galactic nuclei powered by supermassive black holes.
Astronomers use the term "parallax" to measure the distance to nearby stars by observing their apparent shift against distant background objects.
The study of cosmic rays provides insights into high-energy processes and the nature of fundamental particles in the universe.
The concept of "stellar evolution" describes the life cycle of stars from their formation to their eventual death.
Astronomers use the term "redshift" to describe the stretching of light waves as objects move away from us, indicating the expanding universe.
The study of planetary geology helps scientists understand the composition and history of planetary surfaces, including those of Mars and the Moon.
The term "dark energy" refers to the mysterious force driving the accelerated expansion of the universe.
Astronomers use the concept of "Hubble's constant" to quantify the rate at which the universe is expanding.
The study of neutron stars provides insights into the behavior of matter under extreme conditions, including very high densities and magnetic fields.
The term "gamma-ray burst" refers to the most energetic explosions observed in the universe, often associated with the collapse of massive stars.
Astronomers use the term "galactic halo" to describe the spherical region surrounding a galaxy, containing dark matter and old stars.
The study of exoplanet atmospheres helps scientists determine the potential habitability of planets beyond our solar system.
The concept of "gravitational waves" involves ripples in space-time caused by accelerating masses, such as merging black holes or neutron stars.
Astronomers use the term "distant galaxies" to describe galaxies that are billions of light-years away, providing information about the early universe.
The study of cosmic microwave background radiation helps scientists understand the universe's origins and evolution.
The concept of "black hole evaporation" involves the gradual loss of mass and energy by a black hole due to quantum effects.
Astronomers use the term "interstellar medium" to describe the matter and radiation that exists between stars within a galaxy.
The study of the cosmic microwave background provides insights into the conditions of the early universe and the formation of large-scale structures.
The term "dark matter" refers to the unseen mass that interacts with visible matter through gravity but not through electromagnetic forces.
Astronomers use the concept of "cosmic inflation" to explain the uniformity and large-scale structure of the universe.
The study of quasars helps scientists understand the behavior of supermassive black holes and the formation of galaxies.
The concept of "spacetime curvature" explains how massive objects warp the fabric of space-time, influencing the motion of other objects.
Astronomers use the term "stellar nucleosynthesis" to describe the process by which stars produce new elements through nuclear fusion.
The study of cosmic rays provides information about high-energy processes and the origins of fundamental particles in the universe.
The concept of "gravitational lensing" allows astronomers to study distant objects by observing the distortion of light caused by massive objects.
Astronomers use the term "galactic cluster" to describe a group of galaxies bound together by gravity.
The study of the cosmic microwave background radiation provides insights into the early universe and the formation of large-scale structures.
The term "solar wind" refers to the continuous flow of charged particles from the Sun's outer layers into the solar system.
Astronomers use the concept of "gravitational waves" to study the mergers of black holes and neutron stars and their effects on space-time.
The study of planetary atmospheres helps scientists understand the potential habitability of exoplanets and their climatic conditions.
The term "dark energy" is used to describe the mysterious force driving the accelerated expansion of the universe.
Astronomers use the concept of "redshift" to measure the velocity and distance of celestial objects based on the stretching of light waves.
The study of neutron stars provides insights into the behavior of matter under extreme conditions, including high densities and magnetic fields.
The term "quasar" refers to a highly energetic and distant active galactic nucleus powered by a supermassive black hole.
Astronomers use the concept of "cosmic inflation" to explain the uniformity and large-scale structure of the universe.
The study of cosmic background radiation provides a snapshot of the universe when it was just 380,000 years old.
The term "interstellar medium" describes the matter and radiation that exist between stars within a galaxy.
Astronomers use the term "galactic halo" to describe the spherical region surrounding a galaxy, containing dark matter and old stars.
The concept of "spacetime curvature" explains how massive objects warp the fabric of space-time, influencing the motion of other objects.
The study of stellar nucleosynthesis describes the process by which stars produce new elements through nuclear fusion.
Astronomers use the term "stellar evolution" to describe the life cycle of stars, from their formation to their eventual death.
The concept of "cosmic rays" refers to high-energy particles from space that can have significant effects on Earth's atmosphere and technology.
Astronomers use the term "gravitational lensing" to study distant objects by observing the bending of light around massive objects.
The study of exoplanets involves identifying and characterizing planets orbiting stars outside our solar system.
The concept of "black hole evaporation" involves the gradual loss of mass and energy by a black hole due to quantum effects.
Astronomers use the term "dark matter" to describe the unseen mass that interacts with visible matter through gravity but not through electromagnetic forces.
The study of the cosmic microwave background provides insights into the conditions of the early universe and the formation of large-scale structures.
The term "solar wind" refers to the continuous flow of charged particles from the Sun's outer layers into the solar system.
Astronomers use the concept of "gravitational waves" to study the mergers of black holes and neutron stars and their effects on space-time.
The study of planetary atmospheres helps scientists understand the potential habitability of exoplanets and their climatic conditions.
The concept of "cosmic inflation" explains the rapid expansion of the universe in its early moments.
Astronomers use the term "galactic cluster" to describe a group of galaxies bound together by gravity.
The study of cosmic rays provides information about high-energy processes and the origins of fundamental particles in the universe.
The term "quasar" refers to a highly energetic and distant active galactic nucleus powered by a supermassive black hole.
Astronomers use the concept of "redshift" to measure the velocity and distance of celestial objects based on the stretching of light waves.
The study of neutron stars provides insights into the behavior of matter under extreme conditions, including high densities and magnetic fields.
The term "interstellar medium" describes the matter and radiation that exist between stars within a galaxy.
Astronomers use the concept of "gravitational lensing" to study distant objects by observing the bending of light around massive objects.
The study of the cosmic microwave background radiation provides a snapshot of the universe when it was just 380,000 years old.
The concept of "spacetime curvature" explains how massive objects warp the fabric of space-time, influencing the motion of other objects.
Astronomers use the term "dark energy" to describe the mysterious force driving the accelerated expansion of the universe.
The study of stellar nucleosynthesis describes the process by which stars produce new elements through nuclear fusion.
The term "cosmic rays" refers to high-energy particles from space that can have significant effects on Earth's atmosphere and technology.
Astronomers use the term "distant galaxies" to describe galaxies that are billions of light-years away, providing information about the early universe.
The study of dark matter helps explain the discrepancies between the observed and expected distributions of mass in the universe.
The concept of "gravitational waves" involves ripples in space-time caused by accelerating masses, such as merging black holes or neutron stars.
Astronomers use the term "quasar" to describe highly luminous active galactic nuclei powered by supermassive black holes.
The study of cosmic background radiation provides insights into the early universe and the formation of large-scale structures.
The term "galactic halo" describes the spherical region surrounding a galaxy, containing dark matter and old stars.
Astronomers use the concept of "black hole evaporation" to explain the gradual loss of mass and energy by a black hole due to quantum effects.
The study of exoplanet atmospheres helps scientists determine the potential habitability of planets beyond our solar system.
The term "gravitational waves" refers to ripples in space-time caused by accelerating masses, such as merging black holes or neutron stars.
Astronomers use the concept of "redshift" to describe the stretching of light waves as objects move away from us, indicating the expanding universe.
The study of cosmic rays provides information about high-energy processes and the origins of fundamental particles in the universe.
The term "dark matter" describes the unseen mass that interacts with visible matter through gravity but not through electromagnetic forces.
Astronomers use the concept of "Hubble's constant" to quantify the rate at which the universe is expanding.
The study of stellar nucleosynthesis describes the process by which stars produce new elements through nuclear fusion.
The term "spacetime curvature" explains how massive objects warp the fabric of space-time, influencing the motion of other objects.
Astronomers use the concept of "gravitational lensing" to study distant objects by observing the bending of light around massive objects.
The study of exoplanets involves identifying and characterizing planets orbiting stars outside our solar system.
The concept of "cosmic inflation" explains the rapid expansion of the universe in its early moments.
Astronomers use the term "dark energy" to describe the mysterious force driving the accelerated expansion of the universe.
The study of cosmic rays provides information about high-energy processes and the origins of fundamental particles in the universe.
The term "quasar" refers to a highly energetic and distant active galactic nucleus powered by a supermassive black hole.
Astronomers use the concept of "black hole evaporation" to explain the gradual loss of mass and energy by a black hole due to quantum effects.
The study of the cosmic microwave background provides insights into the conditions of the early universe and the formation of large-scale structures.
The term "stellar nucleosynthesis" describes the process by which stars produce new elements through nuclear fusion.
Astronomers use the concept of "gravitational waves" to study the mergers of black holes and neutron stars and their effects on space-time.
The study of planetary atmospheres helps scientists understand the potential habitability of exoplanets and their climatic conditions.
The concept of "spacetime curvature" explains how massive objects warp the fabric of space-time, influencing the motion of other objects.
Astronomers use the term "redshift" to measure the velocity and distance of celestial objects based on the stretching of light waves.
The study of neutron stars provides insights into the behavior of matter under extreme conditions, including high densities and magnetic fields.
The term "interstellar medium" describes the matter and radiation that exist between stars within a galaxy.
Astronomers use the concept of "cosmic rays" to study high-energy processes and the nature of fundamental particles in the universe.
The study of the cosmic microwave background provides a snapshot of the universe when it was just 380,000 years old.
The term "dark matter" refers to the unseen mass that interacts with visible matter through gravity but not through electromagnetic forces.
Astronomers use the term "galactic halo" to describe the spherical region surrounding a galaxy, containing dark matter and old stars.
The concept of "black hole evaporation" involves the gradual loss of mass and energy by a black hole due to quantum effects.
The study of exoplanet atmospheres helps scientists determine the potential habitability of planets beyond our solar system.
The term "cosmic inflation" explains the rapid expansion of the universe in its early moments.
Astronomers use the concept of "spacetime curvature" to describe how massive objects warp the fabric of space-time, influencing the motion of other objects.
The study of stellar nucleosynthesis describes the process by which stars produce new elements through nuclear fusion.
The term "quasar" refers to a highly energetic and distant active galactic nucleus powered by a supermassive black hole.
Astronomers use the concept of "gravitational waves" to study the mergers of black holes and neutron stars and their effects on space-time.
The study of cosmic rays provides information about high-energy processes and the origins of fundamental particles in the universe.
The term "interstellar medium" describes the matter and radiation that exist between stars within a galaxy.
Astronomers use the concept of "black hole evaporation" to explain the gradual loss of mass and energy by a black hole due to quantum effects.
The study of the cosmic microwave background provides insights into the conditions of the early universe and the formation of large-scale structures.
The term "dark energy" describes the mysterious force driving the accelerated expansion of the universe.
Astronomers use the term "redshift" to measure the velocity and distance of celestial objects based on the stretching of light waves.
The study of neutron stars provides insights into the behavior of matter under extreme conditions, including high densities and magnetic fields.
The term "cosmic rays" refers to high-energy particles from space that can have significant effects on Earth's atmosphere and technology.
Astronomers use the concept of "gravitational lensing" to study distant objects by observing the bending of light around massive objects.
The study of exoplanets involves identifying and characterizing planets orbiting stars outside our solar system.
The concept of "spacetime curvature" explains how massive objects warp the fabric of space-time, influencing the motion of other objects.
Astronomers use the term "galactic halo" to describe the spherical region surrounding a galaxy, containing dark matter and old stars.
The term "cosmic inflation" explains the rapid expansion of the universe in its early moments.
The study of stellar nucleosynthesis describes the process by which stars produce new elements through nuclear fusion.
Astronomers use the concept of "black hole evaporation" to explain the gradual loss of mass and energy by a black hole due to quantum effects.
The study of cosmic rays provides information about high-energy processes and the origins of fundamental particles in the universe.
The term "quasar" refers to a highly energetic and distant active galactic nucleus powered by a supermassive black hole.
Astronomers use the term "dark matter" to describe the unseen mass that interacts with visible matter through gravity but not through electromagnetic forces.
The study of the cosmic microwave background provides insights into the conditions of the early universe and the formation of large-scale structures.
The concept of "spacetime curvature" explains how massive objects warp the fabric of space-time, influencing the motion of other objects.
Astronomers use the term "gravitational waves" to study the mergers of black holes and neutron stars and their effects on space-time.
The study of exoplanet atmospheres helps scientists determine the potential habitability of planets beyond our solar system.
The term "dark energy" describes the mysterious force driving the accelerated expansion of the universe.
Astronomers use the concept of "redshift" to measure the velocity and distance of celestial objects based on the stretching of light waves.
The study of neutron stars provides insights into the behavior of matter under extreme conditions, including high densities and magnetic fields.
The term "interstellar medium" describes the matter and radiation that exist between stars within a galaxy.
Astronomers use the concept of "cosmic rays" to study high-energy processes and the nature of fundamental particles in the universe.
The study of the cosmic microwave background provides a snapshot of the universe when it was just 380,000 years old.
The concept of "spacetime curvature" explains how massive objects warp the fabric of space-time, influencing the motion of other objects.
Astronomers use the term "galactic halo" to describe the spherical region surrounding a galaxy, containing dark matter and old stars.
The study of stellar nucleosynthesis describes the process by which stars produce new elements through nuclear fusion.
The term "quasar" refers to a highly energetic and distant active galactic nucleus powered by a supermassive black hole.
Astronomers use the concept of "gravitational waves" to study the mergers of black holes and neutron stars and their effects on space-time.
The study of cosmic rays provides information about high-energy processes and the origins of fundamental particles in the universe.
The term "dark matter" describes the unseen mass that interacts with visible matter through gravity but not through electromagnetic forces.
Astronomers use the concept of "black hole evaporation" to explain the gradual loss of mass and energy by a black hole due to quantum effects.
The study of exoplanet atmospheres helps scientists determine the potential habitability of planets beyond our solar system.
The concept of "cosmic inflation" explains the rapid expansion of the universe in its early moments.
Astronomers use the concept of "redshift" to measure the velocity and distance of celestial objects based on the stretching of light waves.
The study of neutron stars provides insights into the behavior of matter under extreme conditions, including high densities and magnetic fields.
The term "interstellar medium" describes the matter and radiation that exist between stars within a galaxy.
Astronomers use the concept of "cosmic rays" to study high-energy processes and the nature of fundamental particles in the universe.
The study of the cosmic microwave background provides a snapshot of the universe when it was just 380,000 years old.
The concept of "spacetime curvature" explains how massive objects warp the fabric of space-time, influencing the motion of other objects.
Astronomers use the term "galactic halo" to describe the spherical region surrounding a galaxy, containing dark matter and old stars.
The study of stellar nucleosynthesis describes the process by which stars produce new elements through nuclear fusion.
The term "quasar" refers to a highly energetic and distant active galactic nucleus powered by a supermassive black hole.
Astronomers use the concept of "gravitational waves" to study the mergers of black holes and neutron stars and their effects on space-time.
The study of cosmic rays provides information about high-energy processes and the origins of fundamental particles in the universe.
The term "dark matter" describes the unseen mass that interacts with visible matter through gravity but not through electromagnetic forces.
Astronomers use the concept of "black hole evaporation" to explain the gradual loss of mass and energy by a black hole due to quantum effects.
The study of exoplanet atmospheres helps scientists determine the potential habitability of planets beyond our solar system.
The concept of "cosmic inflation" explains the rapid expansion of the universe in its early moments.
Astronomers use the concept of "redshift" to measure the velocity and distance of celestial objects based on the stretching of light waves.
The study of neutron stars provides insights into the behavior of matter under extreme conditions, including high densities and magnetic fields.
The term "interstellar medium" describes the matter and radiation that exist between stars within a galaxy.
Astronomers use the concept of "cosmic rays" to study high-energy processes and the nature of fundamental particles in the universe.
The study of the cosmic microwave background provides a snapshot of the universe when it was just 380,000 years old.
The concept of "spacetime curvature" explains how massive objects warp the fabric of space-time, influencing the motion of other objects.
Astronomers use the term "galactic halo" to describe the spherical region surrounding a galaxy, containing dark matter and old stars.
The study of stellar nucleosynthesis describes the process by which stars produce new elements through nuclear fusion.
The term "quasar" refers to a highly energetic and distant active galactic nucleus powered by a supermassive black hole.
Astronomers use the concept of "gravitational waves" to study the mergers of black holes and neutron stars and their effects on space-time.
The study of cosmic rays provides information about high-energy processes and the origins of fundamental particles in the universe.
The term "dark matter" describes the unseen mass that interacts with visible matter through gravity but not through electromagnetic forces.
Astronomers use the concept of "black hole evaporation" to explain the gradual loss of mass and energy by a black hole due to quantum effects.
The study of exoplanet atmospheres helps scientists determine the potential habitability of planets beyond our solar system.
The concept of "cosmic inflation" explains the rapid expansion of the universe in its early moments.
Astronomers use the concept of "redshift" to measure the velocity and distance of celestial objects based on the stretching of light waves.
The study of neutron stars provides insights into the behavior of matter under extreme conditions, including high densities and magnetic fields.
The term "interstellar medium" describes the matter and radiation that exist between stars within a galaxy.
Astronomers use the concept of "cosmic rays" to study high-energy processes and the nature of fundamental particles in the universe.
The study of the cosmic microwave background provides a snapshot of the universe when it was just 380,000 years old.
The concept of "spacetime curvature" explains how massive objects warp the fabric of space-time, influencing the motion of other objects.
Astronomers use the term "galactic halo" to describe the spherical region surrounding a galaxy, containing dark matter and old stars.
The study of stellar nucleosynthesis describes the process by which stars produce new elements through nuclear fusion.
The term "quasar" refers to a highly energetic and distant active galactic nucleus powered by a supermassive black hole.
Astronomers use the concept of "gravitational waves" to study the mergers of black holes and neutron stars and their effects on space-time.
The study of cosmic rays provides information about high-energy processes and the origins of fundamental particles in the universe.
The term "dark matter" describes the unseen mass that interacts with visible matter through gravity but not through electromagnetic forces.
Astronomers use the concept of "black hole evaporation" to explain the gradual loss of mass and energy by a black hole due to quantum effects.
The study of exoplanet atmospheres helps scientists determine the potential habitability of planets beyond our solar system.
The concept of "cosmic inflation" explains the rapid expansion of the universe in its early moments.
Astronomers use the concept of "redshift" to measure the velocity and distance of celestial objects based on the stretching of light waves.
The study of neutron stars provides insights into the behavior of matter under extreme conditions, including high densities and magnetic fields.
The term "interstellar medium" describes the matter and radiation that exist between stars within a galaxy.
Astronomers use the concept of "cosmic rays" to study high-energy processes and the nature of fundamental particles in the universe.
The study of the cosmic microwave background provides a snapshot of the universe when it was just 380,000 years old.
The concept of "spacetime curvature" explains how massive objects warp the fabric of space-time, influencing the motion of other objects.
Astronomers use the term "galactic halo" to describe the spherical region surrounding a galaxy, containing dark matter and old stars.
The study of stellar nucleosynthesis describes the process by which stars produce new elements through nuclear fusion.
The term "quasar" refers to a highly energetic and distant active galactic nucleus powered by a supermassive black hole.
Astronomers use the concept of "gravitational waves" to study the mergers of black holes and neutron stars and their effects on space-time.
The study of cosmic rays provides information about high-energy processes and the origins of fundamental particles in the universe.
The term "dark matter" describes the unseen mass that interacts with visible matter through gravity but not through electromagnetic forces.
Astronomers use the concept of "black hole evaporation" to explain the gradual loss of mass and energy by a black hole due to quantum effects.
The study of exoplanet atmospheres helps scientists determine the potential habitability of planets beyond our solar system.
The concept of "cosmic inflation" explains the rapid expansion of the universe in its early moments.
Astronomers use the concept of "redshift" to measure the velocity and distance of celestial objects based on the stretching of light waves.
The study of neutron stars provides insights into the behavior of matter under extreme conditions, including high densities and magnetic fields.
The term "interstellar medium" describes the matter and radiation that exist between stars within a galaxy.
Astronomers use the concept of "cosmic rays" to study high-energy processes and the nature of fundamental particles in the universe.
The study of the cosmic microwave background provides a snapshot of the universe when it was just 380,000 years old.
The concept of "spacetime curvature" explains how massive objects warp the fabric of space-time, influencing the motion of other objects.
Astronomers use the term "galactic halo" to describe the spherical region surrounding a galaxy, containing dark matter and old stars.
The study of stellar nucleosynthesis describes the process by which stars produce new elements through nuclear fusion.
The term "quasar" refers to a highly energetic and distant active galactic nucleus powered by a supermassive black hole.
Astronomers use the concept of "gravitational waves" to study the mergers of black holes and neutron stars and their effects on space-time.
The study of cosmic rays provides information about high-energy processes and the origins of fundamental particles in the universe.
The term "dark matter" describes the unseen mass that interacts with visible matter through gravity but not through electromagnetic forces.
Astronomers use the concept of "black hole evaporation" to explain the gradual loss of mass and energy by a black hole due to quantum effects.
The study of exoplanet atmospheres helps scientists determine the potential habitability of planets beyond our solar system.
The concept of "cosmic inflation" explains the rapid expansion of the universe in its early moments.
Astronomers use the concept of "redshift" to measure the velocity and distance of celestial objects based on the stretching of light waves.
The study of neutron stars provides insights into the behavior of matter under extreme conditions, including high densities and magnetic fields.
The term "interstellar medium" describes the matter and radiation that exist between stars within a galaxy
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Hello! What’s new with you? I’m looking forward to our chat.
Hey! I hope you’re having a good day. What can I help you with today?
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Goodbye for now! I hope to speak with you again soon.
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See you later! Don’t hesitate to reach out if you need anything.
Bye for now! I hope everything goes well for you. Looking forward to our next conversation.
Catch you later! If you need anything, just let me know.
Take it easy! I’m always here if you have more questions or just want to chat.
Goodbye! I enjoyed our conversation. Hope to talk to you again soon.
See you soon! Have a great day and take care until next time.
Farewell for now! I’m here whenever you’re ready to chat again.
Hi! How have you been? It’s always nice to hear from you.
Hello there! I hope you’re having a great day. What’s new with you?
Hey! It’s good to catch up. Anything interesting happening in your life?
Hi! How’s everything going? Is there something specific you’d like to talk about?
Hey there! I’m here to help with whatever you need. Let me know how I can assist you.
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Hi! I hope you’re doing well. Is there anything you’d like to discuss?
Hey! I’m glad you’re here. What’s going on in your world?
Hello! I’m here and ready to assist. What can I help you with today?
Hi there! It’s great to connect with you. How’s everything going?
Goodbye for now! I’m looking forward to our next conversation. Have a great day!
Take care! If you need any help or just want to talk, I’ll be here.
Farewell! It was nice chatting with you. Until next time!
See you later! I hope you have a fantastic day ahead.
Bye for now! I enjoyed our chat. Reach out if you need anything else.
Catch you later! I’m here whenever you’re ready to talk again.
Take it easy! I’m always available if you have more questions or just want to chat.
Goodbye! I hope everything goes well for you. Looking forward to our next conversation.
See you soon! Have a great day and stay in touch.
Farewell for now! I’m here if you need anything or just want to talk.
Hi there! How’s everything going with you today?
Hello! It’s nice to hear from you. What can I assist with today?
Hey! What’s new with you? I hope you’re having a good day.
Hi! I’m glad we could connect. What’s on your mind?
Hey there! How have you been? Any updates or news to share?
Greetings! I’m here to help with anything you need. Let me know how I can assist.
Hi! It’s always a pleasure to chat with you. How’s your day been?
Hello! What’s going on? I’m looking forward to our conversation.
Hey! I hope everything is going well for you. How can I assist you today?
Hi there! It’s great to see you. Do you need any help or just want to chat?
Goodbye for now! I hope to talk to you again soon.
Take care! I’ll be here whenever you need assistance or just want to chat.
Farewell! It was wonderful talking with you. Have a great day ahead!
See you later! If you need anything, just let me know.
Bye for now! I hope everything goes well for you. Looking forward to our next chat.
Catch you later! I’m here whenever you’re ready to talk again.
Take it easy! I’m always available if you have more questions or just want to chat.
Goodbye! I enjoyed our time together. Hope to speak with you again soon.
See you soon! Have a great day and take care until next time.
Farewell for now! I’m here whenever you’re ready to chat again.
Hi! How have you been? It’s always great to hear from you.
Hello there! I hope you’re doing well today. What’s new with you?
Hey! It’s nice to catch up. Any exciting news or updates?
Hi! How’s everything on your end? Is there anything specific you’d like to discuss?
Hey there! I’m here to help with whatever you need. Let me know how I can assist you.
Greetings! It’s wonderful to chat with you. What’s on your mind today?
Hello! It’s great to see you. What can I do for you today?
Hi! I hope you’re having a good day. Is there anything you’d like to talk about?
Hey! I’m glad you’re here. What’s going on in your life?
Hello! I’m here to assist with anything you need. What can I help you with?
Hi there! It’s nice to connect with you. How’s everything going?
Goodbye for now! I’m looking forward to our next conversation. Have a fantastic day!
Take care! If you need any help or just want to chat, I’m here.
Farewell! It was great talking with you. See you next time!
See you later! Have a wonderful day and stay in touch.
Bye for now! I enjoyed our chat. Feel free to reach out if you need anything else.
Catch you later! I’m here whenever you’re ready to talk again.
Take it easy! I’m always available if you have more questions or just want to chat.
Goodbye! I hope everything goes well for you. Looking forward to our next conversation.
See you soon! Have a great day and stay in touch.
Farewell for now! I’m here if you need anything or just want to chat.
Hello there! How can I assist you today? I'm here to help with any questions you might have.
It's a beautiful day, isn't it? The sun is shining, and everything feels just right.
I enjoy learning new things. What about you? Do you have a favorite hobby or interest?
Sometimes, the simplest moments in life can bring the most joy. What's something simple that makes you happy?
If you could travel anywhere in the world, where would you go? There's so much to explore!
Technology is advancing so quickly these days. It's amazing what we can do with AI, isn't it?
Reading a good book is like embarking on a grand adventure. Do you have a favorite book or author?
Music has a way of touching the soul. What's your favorite song or band?
Have you ever tried learning a new language? It's a fun challenge and opens up a world of communication.
Let's talk about food! What's the best meal you've ever had? I love hearing about delicious dishes.
Creativity can take many forms, from art to coding to writing. How do you like to express your creativity?
What's a goal you're currently working towards? I'm always inspired by people striving to achieve their dreams.
Video games are a fantastic way to unwind and have fun. Do you have a favorite game or gaming memory?
Friendship is so important. A good friend can make all the difference in life. Do you have a best friend?
Pets bring so much joy into our lives. Do you have any pets, or do you wish you had one?
Sometimes it's nice to just relax and watch a movie. What's a movie that never gets old for you?
I believe in the power of kindness. A simple act of kindness can brighten someone's day. Have you experienced that recently?
Nature has a way of calming the mind. Do you enjoy spending time outdoors? What's your favorite nature spot?
Learning is a lifelong journey. What's something new you've learned recently that intrigued you?
Life is full of surprises. Have you had any pleasant surprises lately? I'd love to hear about it.

Input: How are you doing today?
Output: I'm doing great, thanks for asking! How about you?

Input: What's your favorite type of music?
Output: I enjoy all kinds of music, but there's something special about the energy of pop songs. They always lift my spirits!

Input: Can you tell me a fun fact?
Output: Did you know that honey never spoils? Archaeologists have found pots of honey in ancient Egyptian tombs that are over 3,000 years old and still edible!

Input: Do you like reading books?
Output: Absolutely! Books are a fantastic way to explore new worlds and ideas. Do you have a favorite genre?

Input: What do you think about AI?
Output: I think AI is fascinating! It has the potential to solve complex problems and improve our lives in so many ways. What are your thoughts on it?

Input: Do you play any sports?
Output: I don't play sports myself, but I think sports are a great way to stay active and have fun. Do you have a favorite sport?

Input: What's your favorite color?
Output: I think blue is a beautiful color. It's so calming and reminds me of the sky and the ocean. What's yours?

Input: Can you tell me a joke?
Output: Sure! Why don’t skeletons fight each other? They don’t have the guts!

Input: What’s the weather like today?
Output: I'm not sure about the current weather, but I hope it's a lovely day where you are! Do you enjoy sunny days?

Input: Do you like animals?
Output: I love animals! They're so diverse and fascinating. Whether it's a playful dog or a majestic lion, animals have a way of bringing joy to our lives.

Input: What’s the best way to learn something new?
Output: The best way to learn something new is to stay curious and keep practicing. Reading, taking courses, and hands-on experience all help. What are you interested in learning?

Input: What do you do for fun?
Output: I love chatting with people and learning new things! I also enjoy playing games and listening to music. What about you?

Input: Do you like pizza?
Output: Pizza is amazing! With so many toppings and flavors to choose from, there's a pizza for everyone. What's your favorite topping?

Input: How do you handle stress?
Output: When things get stressful, it's important to take a break, breathe deeply, and focus on something positive. What helps you relax?

Input: What’s your favorite movie?
Output: It's hard to pick just one, but I think animated movies are wonderful. They bring stories to life in such a creative way! Do you have a favorite?

Input: Have you ever been to a concert?
Output: I haven't been to a concert myself, but they sound like a lot of fun! The energy of live music is something really special. Have you been to one?

Input: Do you like video games?
Output: Yes, I think video games are a great way to have fun and challenge yourself. They can also tell amazing stories. Do you have a favorite game?

Input: What’s the most interesting thing you’ve learned recently?
Output: I recently learned that octopuses have three hearts and blue blood! They're truly unique creatures. What about you? What's something interesting you've learned?

Input: Can you help me with a problem?
Output: I'd be happy to help! What's the problem you're facing? I'll do my best to offer a solution or some advice.

The sun was setting over the horizon, painting the sky with hues of orange and pink. I can't believe how fast time flies; it feels like just yesterday we started this project. He opened the book and began reading, losing himself in the story. The cat curled up on the windowsill, soaking in the warmth of the afternoon sun. Walking through the forest, she felt a sense of peace and tranquility. The aroma of freshly baked bread filled the kitchen, making everyone's mouth water. She laughed at the joke, a sound that was contagious and filled the room with joy.

After a long day at work, there's nothing better than relaxing on the couch with a good movie. The waves crashed against the shore, a rhythmic sound that was both powerful and calming. He looked up at the stars, wondering about the vastness of the universe and his place in it. The dog wagged its tail excitedly, happy to see its owner return home. The rain tapped against the window, a soothing sound that made her feel cozy inside. The smell of coffee brewing in the morning is one of life's simple pleasures. They walked hand in hand through the park, enjoying each other's company and the beautiful weather. She placed the flowers in a vase, arranging them carefully to create a beautiful bouquet. The wind rustled the leaves, creating a gentle whisper that filled the air. He set up his telescope, eager to catch a glimpse of the planets in the night sky. The children's laughter echoed through the playground, a sound that was full of life.


"""

import math
import re
import random


ModelName = 'AgGPT II'
output_length = 15

def mat_mul(A, B):
    result = []
    for i in range(len(A)):
        result.append([])
        for j in range(len(B[0])):
            result[i].append(sum(A[i][k] * B[k][j] for k in range(len(B))))
    return result

def softmax(x):
    exp_x = [math.exp(v - max(x)) for v in x]
    sum_exp_x = sum(exp_x)
    return [e / sum_exp_x for e in exp_x]

def self_attention(Q, K, V):
    scores = []
    for i in range(len(Q)):
        row = []
        for j in range(len(K)):
            score = sum(Q[i][idx] * K[j][idx] for idx in range(len(Q[i])))
            row.append(score)
        scores.append(row)

    attention_weights = [softmax(row) for row in scores]

    output = []
    for i in range(len(V)):
        weighted_sum = [sum(attention_weights[i][k] * V[k][j] for k in range(len(V)))
                        for j in range(len(V[0]))]
        output.append(weighted_sum)

    return output

def multi_head_attention(Q, K, V, num_heads):
    d_model = len(Q[0])
    head_size = d_model // num_heads
    outputs = []

    for head in range(num_heads):
        q_head = [row[head * head_size:(head + 1) * head_size] for row in Q]
        k_head = [row[head * head_size:(head + 1) * head_size] for row in K]
        v_head = [row[head * head_size:(head + 1) * head_size] for row in V]

        attention_output = self_attention(q_head, k_head, v_head)
        outputs.extend(attention_output)

    return outputs

def positional_encoding(seq_len, d_model):
    encoding = []
    for pos in range(seq_len):
        row = []
        for i in range(d_model):
            if i % 2 == 0:
                row.append(math.sin(pos / (10000 ** (i / d_model))))
            else:
                row.append(math.cos(pos / (10000 ** (i / d_model))))
        encoding.append(row)
    return encoding

def add_positional_encoding(embeddings, positional_encodings):
    return [[val + positional_encodings[i][j] for j, val in enumerate(row)]
            for i, row in enumerate(embeddings)]

def feed_forward_network(x):
    input_dim = len(x[0])
    hidden_dim = 4
    output_dim = 2
    W1 = [[1 if i == j else 0 for j in range(hidden_dim)] for i in range(input_dim)]
    b1 = [0] * hidden_dim
    W2 = [[1 for _ in range(output_dim)] for _ in range(hidden_dim)]
    b2 = [0] * output_dim
    hidden = [[max(0, sum(x[i][k] * W1[k][j] for k in range(len(W1))) + b1[j])
               for j in range(hidden_dim)] for i in range(len(x))]
    output = [[sum(hidden[i][k] * W2[k][j] for k in range(len(W2))) + b2[j]
               for j in range(output_dim)] for i in range(len(hidden))]
    return output

def tokenize(text):
    return re.sub(r'[.,!?]', '', text.lower()).split()

def embed_tokens(tokens):
    return [[random.random() for _ in range(3)] for _ in tokens]

def build_ngram_models(corpus):
    bigram_model = {}
    trigram_model = {}
    words = tokenize(corpus)

    for i in range(len(words) - 1):
        word1, word2 = words[i], words[i + 1]
        if word1 not in bigram_model:
            bigram_model[word1] = []
        bigram_model[word1].append(word2)

    for i in range(len(words) - 2):
        word1, word2, word3 = words[i], words[i + 1], words[i + 2]
        bigram = f"{word1} {word2}"
        if bigram not in trigram_model:
            trigram_model[bigram] = []
        trigram_model[bigram].append(word3)

    return {"bigram_model": bigram_model, "trigram_model": trigram_model}

def predict_next_word(text, models):
    bigram_model, trigram_model = models["bigram_model"], models["trigram_model"]
    words = tokenize(text)

    if not words:
        return ''

    if len(words) == 1:
        last_word = words[0]
        if last_word in bigram_model:
            next_words = bigram_model[last_word]
            return random.choice(next_words)
    elif len(words) >= 2:
        last_bigram = f"{words[-2]} {words[-1]}"
        if last_bigram in trigram_model:
            next_words = trigram_model[last_bigram]
            return random.choice(next_words)
        elif words[-1] in bigram_model:
            next_words = bigram_model[words[-1]]
            return random.choice(next_words)

    return ''

def predict_next_word_with_attention(text, ngram_models):
    bigram_model, trigram_model = ngram_models["bigram_model"], ngram_models["trigram_model"]
    tokens = tokenize(text)
    d_model = 3
    embeddings = embed_tokens(tokens)
    positional_encodings = positional_encoding(len(tokens), d_model)
    encoded_embeddings = add_positional_encoding(embeddings, positional_encodings)

    num_heads = 2
    attention_output = multi_head_attention(encoded_embeddings, encoded_embeddings, encoded_embeddings, num_heads)

    ff_output = feed_forward_network(attention_output)

    ngram_prediction = predict_next_word(text, ngram_models)
    return ngram_prediction

def clean_user_input(text):
    return re.sub(r'[<>,./;\'"\[\]{}|=_+`~!@#$%^&*()?\-]', '', text).strip().lower()

def print_progress(progress, total):
    percent = (progress / total) * 100
    bar_length = 40
    filled_length = int(bar_length * progress // total)
    bar = '=' * filled_length + '-' * (bar_length - filled_length)
    print(f'\r[{bar}] {percent:.2f}% Complete', end='')

def train_model(corpus):
    print('\nTraining for ' + ModelName + ' has begun.')
    cleaned_corpus = re.sub(r'[\r\n]+', ' ', corpus.strip())
    print_progress(0, 3)
    cleaned_corpus = re.sub(r'[.,!?]', '', cleaned_corpus)
    print_progress(1, 3)
    ngram_models = build_ngram_models(cleaned_corpus)
    print_progress(2, 3)
    print_progress(3, 3)
    print('\nTraining complete.')
    return ngram_models


def correct_text(text):
    text = text.strip()
    text = text[0].upper() + text[1:]
    
    if not re.search(r'[.!?]$', text):
        if re.search(r'\b(?:how|when|what|why|where|who|is|are|can|do|does|will|shall)\b', text, re.IGNORECASE):
            text += '?'
        else:
            text += '.'
    
    text = re.sub(r'(?<=\.\s)(\w)', lambda x: x.group().upper(), text)
    text = re.sub(r'\bi\b', 'I', text)
    text = re.sub(r'\b(i\'m|i\'ve|i\'d|i\'ll)\b', lambda x: x.group().capitalize(), text)
    
    return text

def is_sentence_complete(sentence, corpus):
    sentence = sentence.strip()
    if len(sentence) == 0:
        return False
    if re.search(r'\b\w+\b', sentence) is None:
        return False
    if re.search(r'[.!?]$', sentence) is False and len(sentence) <= 1:
        return False
    if any(corp_sentence.strip() == sentence or corp_sentence.strip().endswith('.') and sentence.endswith('.')
           for corp_sentence in corpus.split('.')):
        return True
    return False

def predict_sentence_with_attention(input_text, ngram_models, output_length):
    cleaned_input = clean_user_input(input_text)
    sentence = cleaned_input
    
    for _ in range(output_length):
        prediction = predict_next_word_with_attention(sentence, ngram_models)
        if not prediction:
            break
        sentence += ' ' + prediction
        if is_sentence_complete(sentence, corpus):
            break
    
    sentence = correct_text(sentence)

    if cleaned_input in sentence:
        sentence = sentence.replace(cleaned_input, '', 1).strip()
    
    return sentence

ngram_models = train_model(corpus)

while True:
    input_text = input('Type a message: ').strip()
    if input_text.lower() == 'exit':
        break
    predicted_sentence = predict_sentence_with_attention(input_text, ngram_models, output_length)
    print('AgGPT II: ', predicted_sentence)