Relativity and c/sqrt{3}
| dc.creator | Blinnikov, S. I. | |
| dc.creator | Okun, L. B. | |
| dc.creator | Vysotsky, M. I. | |
| dc.date | 2001-11-29 | |
| dc.date | 2001-12-28 | |
| dc.date.accessioned | 2026-07-07T03:26:29Z | |
| dc.date.available | 2026-07-07T03:26:29Z | |
| dc.description | We define the critical coordinate velocity v_c. A particle moving radially in Schwarzschild background with this velocity, v_c= c/sqrt 3, is neither accelerated, nor decelerated if gravitational field is weak, r_g << r, where r_g is the gravitational radius, while r is the current one. We find that the numerical coincidence of v_c with velocity of sound in ultrarelativistic plasma, u_s, is accidental, since two velocities are different if the number of spatial dimensions is not equal to 3 | |
| dc.description | 6 pages; PS with an essential reference added. Contribution to Holger Nielsen festschrift | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0111103 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0111103 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/34061 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | Astrophysics | |
| dc.subject | Classical Physics | |
| dc.title | Relativity and c/sqrt{3} | |
| dc.type | text |