P C W Davies 1975 J. Phys. A: Math. Gen. 8 609 doi:10.1088/0305-4470/8/4/022
P C W Davies
Show affiliationsThe procedure used recently by Hawking (1975) to demonstrate the creation of massless particles by black holes is applied to the Rindler coordinate system in flat space-time. The result is that an observer who undergoes a uniform acceleration kappa apparently sees a fixed surface radiate with a temperature of kappa /2 pi . Some implications of this result are discussed.
04.70.-s Physics of black holes
Issue 4 (April 1975)
P C W Davies 1975 J. Phys. A: Math. Gen. 8 609
David S. Graff and Andrew P. Gould 2000 ApJ 534 L51
H. Kishimoto et al 2005 Nucl. Fusion 45 986
Wolfgang Lange and Jean-Michel Gerard 2004 J. Opt. B: Quantum Semiclass. Opt. 6 117
Ramón Escobedo et al 2009 New J. Phys. 11 013033
Álvaro Perales et al 2004 Nanotechnology 15 S229
X George Xu et al 2008 Phys. Med. Biol. 53 R193
K T Tsen et al 2007 J. Phys.: Condens. Matter 19 472201
Thomas Scheidl et al 2009 New J. Phys. 11 085002
Andrzej Olszewski et al 2002 J. Phys. G: Nucl. Part. Phys. 28 1801