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PPT - University of Arizona
PPT - University of Arizona

... For Thomson scattering of photons off of free electrons, assuming the gas is completely ionized and pure hydrogen Other sources of absorption opacity, if present, will contribute to ...
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Neutron Stars and Black Holes
Neutron Stars and Black Holes

... awe, uncertainty, and bad science fiction •! Many people think that black holes are dangerous –! That they suck matter in like “cosmic vacuums” •! Black holes follow the same laws of gravity as everything else ...
Cosmology and Astrophysics II
Cosmology and Astrophysics II

... neither decays nor combines easily to form heavier nuclei. So out of every 16 nucleons (2 neutrons and 14 protons), 4 of these (25%) combined into one helium-4 nucleus. One analogy is to think of helium-4 as ash, and the amount of ash that one forms when one completely burns a piece of wood is insen ...
Linking Asteroids and Meteorites through Reflectance Spectroscopy
Linking Asteroids and Meteorites through Reflectance Spectroscopy

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Black holes Notes

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Black Holes - Gresham College
Black Holes - Gresham College

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Do not mess with time: Probing faster than light travel and

... example, think of the causal loops where at some point ones travels back in time to give to his/her past-self the numbers associated to some lottery. Several solutions have been proposed for such paradoxes (see e.g. for a detailed discussion Ref. 1) we shall here focus on the so called Hawking’s chr ...
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Gravitational Waves – detectors, sources & science

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Hawking radiation



Hawking radiation is black body radiation that is predicted to be released by black holes, due to quantum effects near the event horizon. It is named after the physicist Stephen Hawking, who provided a theoretical argument for its existence in 1974, and sometimes also after Jacob Bekenstein, who predicted that black holes should have a finite, non-zero temperature and entropy.Hawking's work followed his visit to Moscow in 1973 where the Soviet scientists Yakov Zeldovich and Alexei Starobinsky showed him that, according to the quantum mechanical uncertainty principle, rotating black holes should create and emit particles. Hawking radiation reduces the mass and energy of black holes and is therefore also known as black hole evaporation. Because of this, black holes that lose more mass than they gain through other means are expected to shrink and ultimately vanish. Micro black holes are predicted to be larger net emitters of radiation than larger black holes and should shrink and dissipate faster.In September 2010, a signal that is closely related to black hole Hawking radiation (see analog gravity) was claimed to have been observed in a laboratory experiment involving optical light pulses. However, the results remain unverified and debatable. Other projects have been launched to look for this radiation within the framework of analog gravity. In June 2008, NASA launched the Fermi space telescope, which is searching for the terminal gamma-ray flashes expected from evaporating primordial black holes. In the event that speculative large extra dimension theories are correct, CERN's Large Hadron Collider may be able to create micro black holes and observe their evaporation.
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