Probing Black-Hole Physics in the Laboratory Using High Intensity Femtosecond Lasers

Simple item page
dc.creatorSchäfer, G.
dc.creatorSauerbrey, R.
dc.date1998-05-08
dc.date.accessioned2026-07-07T02:26:52Z
dc.date.available2026-07-07T02:26:52Z
dc.descriptionIt is shown how laboratory experiments performed with high intensity femtosecond lasers can probe the physics of black holes in the near-horizon regime. The acceleration generated by the high intensity laser ranging from $10^{13}$g to more than $10^{18}$g is identified with the gravitational acceleration at stretched horizons. In the black-hole's asymptotic region, the stretched-horizon-reflected light shows a measurable universal phase acceleration of $c^4/4GM$. PACS numbers: 04.70.Bw, 97.60.Lf, 52.40.Nk, 52.50.Jm
dc.description15 pages, 4 figures included (psfig used), LateX-209, e-mail: gos@tpi.uni-jena.de, sauerbrey@qe.physik.uni-jena.de
dc.identifierhttps://arxiv.org/abs/astro-ph/9805106
dc.identifierhttp://arxiv.org/abs/astro-ph/9805106
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12454
dc.subjectAstrophysics
dc.titleProbing Black-Hole Physics in the Laboratory Using High Intensity Femtosecond Lasers
dc.typetext

Files

Collections

arXiv