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The Stars education kit - Student activities 11-20
The Stars education kit - Student activities 11-20

Scientific Evaluation of Aulterra`s cell phone neutralizer
Scientific Evaluation of Aulterra`s cell phone neutralizer

... superimposed fields. The first report of such an interaction demonstrated that a secondary crossbeam of visible light could neutralize the biological effects (induction of glutamate-pyruvate-transaminase activity by pretreatment of the substrate alanine) produced by a primary beam of visible light ...
Black Hole Math - Ontario Science Centre
Black Hole Math - Ontario Science Centre

Slide 1
Slide 1

... Matter closer to the center of the disk is traveling faster than matter further from the disk… This causes viscous drag between the inner and outer parts of the disk. The inner disk to loses angular momentum and falls into the central mass. To conserve the total angular momentum it is believed that ...
Notes HERE
Notes HERE

... Space Travel Near Black Holes A probe nearing the event horizon of a black hole will be seen by observers as experiencing a dramatic redshift as it gets closer, so that time appears to be going more and more slowly as it approaches the event horizon. This is called a gravitational redshift – it is ...
transcript.
transcript.

... NEIL DEGRASSE TYSON: Black holes are certainly odd beasts in the universe. They were thought to be peculiar, so peculiar as to, perhaps, not even really exist in the real world. Simply because your equations show that they can exist doesn't require that the real universe has them. ...
The impact of X-rays on molecular cloud fragmentation and the IMF
The impact of X-rays on molecular cloud fragmentation and the IMF

... the impact of X-rays. Simulation B has a cloud near an inactive black hole and has isothermal conditions, with an equation of state of the form P ∝ ρ. The XDR code that updates the thermodynamics is only linked with simulation A where we do have Xrays. The 107 M¯ black hole, at 10% of Eddington, yie ...
Active Galactic Nuclei
Active Galactic Nuclei

... Since quasars can be seen 90% of the way across the universe, they allow us to detect gas throughout the universe. We can therefore examine galaxies (and proto-galaxies) that we can’t even see! Any time the light from a quasar goes through a galaxy that has hydrogen gas, there will be absorption at ...
Black Holes and the Decay of the Universe
Black Holes and the Decay of the Universe

... increases relative to r due to the curved geometry of the black hole. This adjusts the Coleman argument meaning that the bubble forms at smaller radius, and with smaller action. ...
Full text in PDF form
Full text in PDF form

... Formula (10) coincides with (1), nevertheless the problem to calculate the proportionality coecient b requires a special discussion. We have to distinguish between derivation of entropy bound by black hole and eld theory arguments. The bound derived using black hole arguments represent the maximum ...
Gravity - faculty.ucmerced.edu
Gravity - faculty.ucmerced.edu

Astrophysics from radio
Astrophysics from radio

... • Gaia will find some – (Talk by Francois Finet) • What can it tell is about known systems? – Micro-lensing. Stars in the lensing galaxy will lens compact regions (e.g. the AGN) in the lensed objects giving rise to uncorrelated variations in lensed images. This is seen. Gaia will have right cadence ...
Kondo effect of an antidot in the integer quantum Hall regime: a
Kondo effect of an antidot in the integer quantum Hall regime: a

... polarization is equivalent to increasing electron spin polarization. However, this result does not match those expected in the experiment [8] of large-size realistic antidots and the results of the capacitive interaction model [12]. In large-size antidots, it is naturally expected that the spin pola ...
Full PDF
Full PDF

Reprint
Reprint

... evolved stars. Many AGN produce powerful col- ...
microquasars
microquasars

Assignment 10
Assignment 10

... ____ 21. Today, astronomers find compelling evidence that the energy source of the quasars and active galaxies is a. antimatter and matter colliding at the center of a galaxy b. chain reactions of supernova explosions c. matter falling toward a supermassive black hole at the center of a galaxy d. t ...
Goal: To get to know the ins and outs of relativity
Goal: To get to know the ins and outs of relativity

10.2 Galaxies
10.2 Galaxies

... A Star is Born • If the nebula cloud is massive enough, gravity within the cloud will be large enough to shrink it and to raise its temperature above 10 000 000 degrees celsius, a temperature at which atomic fusion happens, releasing huge amounts of energy in the form of all kinds of electromagneti ...
Another version - Scott Aaronson
Another version - Scott Aaronson

... complexity to fundamental physics ...
gr-qc/9409015 DO WE UNDERSTAND BLACK HOLE ENTROPY
gr-qc/9409015 DO WE UNDERSTAND BLACK HOLE ENTROPY

... and semiclassically evolving one, is endowed with an entropy (throughout I use units with G = c= k, but display h) Sf)l¡ = A/(4h) ...
Gravitation, the Quantum, and Cosmological Constant
Gravitation, the Quantum, and Cosmological Constant

... We have seen the emergence of the Bekenstein formula [4] for the black hole entropy from the hypothesis about the microscopic nature of gravitational phenomena. It should be noticed that exactly in the same way as the light quanta [1] have emerged from the Wien black body radiation formula, the nece ...
main sequence
main sequence

... as seen by an observer on Earth, normalized to the value it would have in the absence of the atmosphere. » The brighter the object appears, the lower the value of its ...
Discover - Astronomy Magazine
Discover - Astronomy Magazine

Collapse of an unstable Neutron Star to a Black Hole
Collapse of an unstable Neutron Star to a Black Hole

... Figure 3: Visualization of the (3+1)-formulation are shifted on the spatial slice if the fluid parof general relativity (picture reference: [21]). ticle moves an infinitesimal time step further (see figure 3). By inserting the metric (6) into the Einstein equation one can reformulate the equations i ...
< 1 ... 12 13 14 15 16 17 18 19 20 ... 55 >

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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