2006/07/31 by Hristu Culetu · 1 citation
Physics and Astronomy · #Cosmology and Gravitation Theories #Noncommutative and Quantum Gravity Theories #Relativity and Gravitational Theory #gr-qc #hep-th
paper · pdf · doi:10.1142/s0218271806009601
published as Int.J.Mod.Phys.D15:2177-2180,2006 · 3 pages, revised version, to be published in IJMPD journal
openalex publication_date 2006/12/01 · arxiv created 2006/12/04 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
A nonvanishing value for the Rindler horizon energy is proposed, by an analogy with the "near horizon" Schwarzschild metric. We show that the Rindler horizon energy is given by the same formula E = α/2 obtained by Padmanabhan for the Schwarzschild space–time, where α is the gravitational radius.