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How Black Holes Form in High Energy Collisions Demand Kaloper1 and John Terning2 Department of Physics, University of California, Davis, CA 95616 ABSTRACT We elucidate how black holes form in trans-Planckian

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How to fill out how black holes form:

1. Black holes form from the remnants of massive stars that have exhausted their nuclear fuel and undergo a gravitational collapse.
2. As the star collapses, its enormous mass causes an intense gravitational pull that is so strong that nothing can escape its gravitational grip, not even light.
3. The region of space where the collapsed star's mass is concentrated is called the singularity, and it is surrounded by an event horizon - a boundary beyond which nothing can return.
4. The formation of black holes is intricately linked to the theory of general relativity proposed by Albert Einstein, as it describes the bending of spacetime due to gravitational forces.

Who needs to know how black holes form:

1. Astronomers and astrophysicists: Understanding the formation of black holes is crucial for studying the life cycle of stars, the structure of galaxies, and the evolution of the universe.
2. Researchers and scientists: Knowledge about how black holes form can provide insights into the fundamental properties of matter, gravity, and the nature of spacetime.
3. Space agencies and astronomers: This information helps in designing and conducting observational missions and experiments that aim to detect and study black holes.
4. The general public: Learning about black hole formation fosters scientific curiosity and promotes a deeper understanding of the universe we live in.

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A black hole forms when a massive star collapses under the weight of its own gravity.

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The purpose of studying how black holes form is to gain a better understanding of the universe's evolution and the physics of extreme gravitational forces.

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