New Developments in Black Hole ResearchA black hole is a point of extreme mass in space-time with a radius, or event horizon, inside of which all electromagnetic radiation (including light) is trapped by gravity. A black hole is an extremely compact object, collapsed by gravity which has overcome electric and nuclear forces. It is believed that stars appreciably larger than the Sun, once they have exhausted all their nuclear fuel, collapse to form black holes: they are "black" because no light escapes their intense gravity. Material attracted to a black hole, though, gains enormous energy and can radiate part of it before being swallowed up. Some astronomers believe that enormously massive black holes exist in the centre of our galaxy and of other galaxies. This book brings together leading research from throughout the world. |
Contents
1 | |
TEV BLACK HOLE PRODUCTION BY HIGH ENERGY COSMIC RAYS | 45 |
INTERSECTION OF BLACK HOLE THEORY AND QUANTAM CHROMODYNAMICS THE GLUON PROPAGATOR CORRESPONDING TO LI... | 67 |
ACCRETION ONTO SUPERMASSIVE BLACK HOLES IN QUASARS LEARNING FROM OPTICALUV OBSERVATIONS | 123 |
ENERGY BRIEF HISTORY OF BLACKHOLES AND HAWKINGS UNIVERSE | 185 |
INDEX | 203 |
Common terms and phrases
accretion AGNs air showers Appendix Baldwin effect becomes black hole broad calculated central collapse component condition confining considered consistent constant continuum coordinates correlation corresponding cosmic rays density dependence described Dirac disk distance Eddington effect emission energy equations estimate existence expected extreme factor Fell flow flux functions FWHM(HẞBC GBHC given gluon gravitational gravitational collapse increase inner disk inside limit linear luminosity magnetic field mass matter measurements MECO metric neutrino objects observed obtained operator optical pair parameter particle photon Phys physical possible pressure produce propagator properties quasars quiescent radiation radius range ratio redshift region relation relativistic require shift shown solutions sources spectral spectrum strong structure suggest surface Universe values variability width x-ray
Popular passages
Page 123 - Is set off on the sight, the angle between the line of sight and the axis of the...
Page 61 - B 436, 257 (1998) [arXiv:hep-ph/9804398]. [5] For a review see eg I. Antoniadis, Prepared for NATO Advanced Study Institute and EC Summer School on Progress in String, Field and Particle Theory, Cargese, Corsica, France (2002); and references therein.
Page 172 - Kaspi, S.. Smith, PS. Netzer, H.. Maoz, D.. Jannuzi, BT. & Giveon. U.
Page 43 - The University of Chicago, 5640 S. Ellis Avenue, Chicago, IL 60637, USA...
Page 63 - R. Emparan, GT Horowitz and RC Myers, Phys. Rev. Lett. 85, 499 (2000) [arXiv:hepth/0003118]; A.
Page 38 - RE 1995, in X-ray Binaries, eds. W. Lewin, J. van Paradijs, & E. van den Heuvel, (Cambridge Univ. Press: Cambridge) p 175 63.
Page 171 - Kukula, MJ, Dunlop, JS, McLure, RJ, Miller, L., Percival, WJ, Baum, SA, & O'Dea, CP...
Page 52 - J ,,,..-] , .,,,.1 ,,,,,j io9 .o10 io11 io12 io13 io14 io15 io16 io17 io18 io19 io20 io21 Energy (eV) Figure 3: Cosmic ray flux spectrum.
Page 174 - I. 2003, ASP Conf. Ser. 290, Active Galactic Nuclei: From Central Engine to Host Galaxy, (San Francisco: ASP).