Persuasive Essay On Black Holes

Black holes are one of the most unique mysteries of the universe. The debate as to whether they exist is still taking place many years after the first predictions took place. Cosmologists have known about the possibility of black holes for decades now, but still have no general consensus about what happens to the matter in a black hole once it becomes part of the singularity. Years have been spent researching and learning about them, but without being able to test hypotheses on actual black holes, we really don’t know where the mass goes or what happens next. The best plan right now is to try and create a black hole in a new and bigger particle accelerator. To do this, scientists must first observe elementary particles like neutrinos and gravitons

This knowledge is very crucial to understanding the complex environment that leads to black holes. It all began in 1915 when Einstein first published his paper on the aforementioned relativity theory. Einstein’s new revolutionary theory would be used in the upcoming decades to make bold predictions that most in the scientific community were skeptical about. One of the ideas that Einstein came across was black holes. His research led him to predict they could occur in the universe. However, he thought the idea that matter could be condensed into an infinitely dense point inside these objects was absurd and for the rest of his life rejected this idea, calling it his “biggest mistake.” In the years following his death, physicists would make significant progress on the mathematical formulas and ideas that would lead to an understanding of black holes showing they were

Cosmic H-1 clouds is where the black hole formation process begins (1p59) Then gravity takes over slowly pulling the unstable cloud together. Once stellar equilibrium is achieved, where the interior pressure of the gas cloud equals the force of gravity, a star is born (1p53) For smaller stars like our sun and smaller, made of hydrogen atoms, they cool off once all the hydrogen is gone. Their pressure decreases as they expand turning into red giants. To stay in equilibrium, the star becomes very dense, essentially turning into a whit dwarf star. BOOK 1 sates “This dense pressure results from the kinetic energy of electrons called the Pauli exclusion principal saying no two electrons can occupy the same quantum state” Now with more massive stars, many times larger than our sun, once they deplete their fuel in their core there is no way for them to achieve equilibrium, so they explode violently creating a supernova. The star collapses in on itself propelling part of its mass outward into space, which then forms a nebula around the resultant neutron star. But before they collapse, they start to spin very rapidly, never exceeding the speed of light, therefore becoming a pulsar star. Once the collapse begins, the star’s rotational energy and velocity change as well as having an increased magnetic field (1p90) Pulsars have rotating dipole fields that emit electromagnetic waves slowing its spin (1p91) Once