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Particle detectors in Rindler and Schwarzchild space-times

K J Hinton

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It is shown that a particle detector coupled to the derivative of a scalar quantum field can be viewed as a bona fide 'particle detector'. The response of such a detector is compared with that of a linearly coupled monopole (DeWitt) detector when both are placed in each of three situations; an isotropic particle bath, in Rindler space, and in Schwarzschild space. From their responses it is shown that there is a fundamental difference in how these two detectors behave. As a result, the use of particle detectors to support the close links between quantum field theory in non-Minkowskian spaces and thermal physics is shown to be in need of deeper consideration as is the general role of particle detectors in this theory.


PACS

04.62.+v Quantum fields in curved spacetime

04.70.-s Physics of black holes

MSC

83C47 Methods of quantum field theory (See also 81T20)

81T20 Quantum field theory on curved space backgrounds

83C57 Black holes

Subjects

Gravitation and cosmology

Dates

Issue 9 (21 June 1983)



  1. Particle detectors in Rindler and Schwarzchild space-times

    K J Hinton 1983 J. Phys. A: Math. Gen. 16 1937

  2. Notes on 'particle detectors'

    P G Grove and A C Ottewill 1983 J. Phys. A: Math. Gen. 16 3905

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    J S Dowker 1977 J. Phys. A: Math. Gen. 10 115

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    S A Fulling 1977 J. Phys. A: Math. Gen. 10 917

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    B R Iyer and A Kumar 1980 J. Phys. A: Math. Gen. 13 469

  6. Acceleration radiation in a compact space

    E J Copeland et al 1984 Class. Quantum Grav. 1 179

  7. On an inertial observer's interpretation of the detection of radiation by linearly accelerated particle detectors

    P G Grove 1986 Class. Quantum Grav. 3 801

  8. Is acceleration radiation isotropic?

    P G Grove and A C Ottewill 1985 Class. Quantum Grav. 2 373

  9. Why does an accelerated detector click?

    T Padmanabhan 1985 Class. Quantum Grav. 2 117

  10. On the detection of particle and energy fluxes in two dimensions

    P G Grove 1986 Class. Quantum Grav. 3 793

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