1975
DOI: 10.1088/0305-4470/8/4/022
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Scalar production in Schwarzschild and Rindler metrics

Abstract: Abstract. The procedure used recently by Hawking 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 K apparently sees a fixed surface radiate with a temperature of ~/27t. Some implications of this result are discussed.

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Cited by 901 publications
(795 citation statements)
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References 3 publications
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“…Therefore, the observer must trace over the modes in inaccessible region, losing information about the state, which essentially results in the detection of a thermal state. This effect is called the Unruh effect [33,34]. We consider the following maximally entangled GHZ state …”
Section: Tripartite State In Accelerated Framesmentioning
confidence: 99%
“…Therefore, the observer must trace over the modes in inaccessible region, losing information about the state, which essentially results in the detection of a thermal state. This effect is called the Unruh effect [33,34]. We consider the following maximally entangled GHZ state …”
Section: Tripartite State In Accelerated Framesmentioning
confidence: 99%
“…The state is chosen to be entangled as the GHZ state or the W state. Then switching to the Rindler coordinates for the accelerated observers, we investigate the change of entanglement caused by the Unruh effect [18]. We use the logarithmic negativity as a measure to evaluate the entanglement.…”
Section: Introductionmentioning
confidence: 99%
“…These radiation reaction forces on moving bodies may appear even in the case of only one moving wall [9]- [11]. Connections between the dynamical Casimir effect and several interesting phenomena such as the Unruh-Davies effect [12], black hole physics [13], sonoluminescence [14], mass corrections [15] and quantum decoherence [16] have been discussed in the literature [17].…”
Section: Introductionmentioning
confidence: 99%