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

More documents

Recommendations

Info

Properties of 4D Black HolesPrice ‘72 et all“Black holes have no hair”: Mass, electriccharge and angular momentum are the only 3parameters which specify a stationary BH inEinstein-Maxwell theory (Wheeler, 1971)
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 19 and 20: Uniqueness theorem: Stationary isol
Page 21 and 22: Final state of matter evolutionExot
Page 23 and 24: 40 YEARS LATER …
Page 25: BH theoremsHigher Dim. BHsExact sol
Page 28 and 29: Higher dimensional gravity is stron
Page 30 and 31: "To think that LHC particle collisi
Page 32 and 33: 5D vac. stationary black holes
Page 34 and 35: Complete integrability of geodesic
Page 37 and 38: Existence of the innermost stable c
Page 39 and 40: Gravitational perturbations of a bl
Page 41 and 42: StephenHawking(1942 --)In 1974 Brit
Page 43 and 44: cPlanck units: 105g,PlGcGG10 , 10
Page 46 and 47: Black holes have very high efficien
Page 48 and 49: More than 20 stellar mass BHsobserv
Page 50 and 51: Newtonian mechanics is used to dete
Page 52 and 53: BH as a classical object: M 105gPri
Page 55 and 56: Stars in Keplerian orbits around ce
Page 57 and 58: Tidal disruption of a star at close
Page 60 and 61: CollapseEvaporation Pure Black T
Page 62 and 63: String theoryAdF/CFTLoop gravityBH
Page 64 and 65: plays the roleof time inside BHSlic
Page 67 and 68:
Birth: Matter is generated during t
show all

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

You also want an ePaper? Increase the reach of your titles

Delete template?

Save as template?