Ginzburg Conference on Physics May 28 - June 2, 2012 in Moscow

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The vacuum near a black hole is unstable.The gravitational field is so strong that itproduces particles. As a result the black holeemits as a heated black body with temperature:kTc3106MK8GM M
cPlanck units: 105g,PlGcGG10 , 10 secc33 cm 433 Pl 5Life-time of a black hole:tBH3 3 M M 17 10 secPl 1015 g Pl Hawking effect is important for mini-black-holes only
Page 1: Ginzburg C
Page 4: Black hole concept,its evolution,mo
Page 7 and 8: Black hole gravity is strong:2 2GMc
Page 9 and 10: GRAVITY1 8MATTERR g R T 2 c4 MATT
Page 11 and 12: Black Holes vs Dark Starts“Nature
Page 13 and 14: JohnArchibaldWheeler(1911--2008)The
Page 15: In 60’-70’th of the past centur
Page 18 and 19: Event horizon (BH boundary) is almo
Page 20 and 21: Massless field equations allow the
Page 22 and 23: R.I.P.Black Holes as Graves of Matt
Page 24 and 25: At: http://www.google.caBLACK HOLE
Page 27 and 28: Motivations :(1) Extra-dimensions a
Page 29 and 30: New fundamental (quantum gravity) s
Page 31 and 32: If in D-dimensional ST there exist
Page 33 and 34: (1) No Uniquness Theorem: For given
Page 35: All Kerr-NUT-AdS metrics possess a
Page 38 and 39: Schwarzschild BH:r 3r 6MISCOEISCOg/
Page 40 and 41: Bekenstein 72-73, Hawking74-75dMAS
Page 44: Equivalenceprinciple inquantum doma
Page 47 and 48: Total number of stars in our Galaxy
Page 49 and 50: Persistent BHs ( Syg X 1, LMC X 1,
Page 51 and 52: Gamma-ray bursts (GRB) are the brig
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Page 65: “Through A Black Hole Into A New
Page 68: http://www.amazon.ca/Introduction-B

Ginzburg Conference on Physics May 28 - June 2, 2012 in Moscow

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