Gravity: An Introduction to Einstein's General Relativity

By J. Fabris. 2004

700 citations recorded by the source corpus.

Subfields: Artificial Intelligence, Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/68b1b5b029e85b327b24f4ab510aebc2d469b939

How researchers see this paper

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In Artificial Intelligence

1. V. Kagramanova
2. Jutta Kunz
3. C. Cattoën
4. Matt Visser
5. E. Flanagan
6. S. Horiuchi
7. J. Kneller
8. S. Hughes

In Astronomy and Astrophysics

1. Cosimo Bambi
2. C. Cattoën
3. E. Flanagan
4. S. Hughes
5. Matt Visser
6. V. Kagramanova
7. G. Giribet
8. Jutta Kunz

Citations in the corpus

• Black holes in astrophysics (2005, background): “In contrast, systems like A0620–00 and other X-ray novae have low-mass companions which often have masses less than 10 percent of M .”
• Solar system effects in Schwarzschild de Sitter space time (2006, background): “An observer moving with the gyroscope on a circular orbit in the equatorial plane will see its spin precess in the equatorial plane, see e.g. [ 14 ].”
• The basics of gravitational wave theory (2005, background): “New Journal of Physics 7 (2005) 204 PII: S1367-2630(05)92710-9 1367-2630/05/010204+51$30.00 © IOP Publishing Ltd and Deutsche Physikalische Gesellschaft Contents”
• What can be learned from a future supernova neutrino detection (2017, background): “Interestingly general relativistic effects prevent the spike in luminosity from being as large as it could be: when the neutrinosphere is below the photon sphere— the radius where massless particles can orbit a gravitational source—only neutrinos emitted within a narrow cone of the radial direction ”
• The Kerr spacetime: A brief introduction (2007, background): “The final form of Albert Einstein’s general theory of relativity was developed in November 1915 [3, 4], and within two months Karl Schwarzschild (working with one of the slightly earlier versions of the theory) had already solved the field equations that determine the exact spacetime geometry of a…”
• Hawking radiation, the Stefan–Boltzmann law, and unitarization (2015, neutral): “[8]) for a classical massless particle.”
• Necessary and sufficient conditions for big bangs, bounces, crunches, rips, sudden singularities and extremality events (2005, background): “However, over the last few years, the zoo of cosmological singularities considered in the literature has become considerably more extensive, with “big rips” and “sudden singularities” added to the mix, as well as renewed interest in non-singular cosmological events such as “bounces” and…”
• Null geodesics and shadow of a rotating black hole in extended Chern-Simons modified gravity (2010, background): “which is the effective potential associated with Kerr solution, to second order in a, as expected (see, for example, [27]).”