Published October 28, 2016 | Version v1
Journal article

Hawking versus Unruh effects, or the difficulty of slowly crossing a black hole horizon

  • 1. Departamento de Astronomía Extragaláctica, Instituto de Astrofísica de Andalucía (CSIC),Glorieta de la Astronomía s/n, 18008 Granada (Spain)
  • 2. Quantenoptik, Quantennanophysik und Quanteninformation, Fakultät für Physik,Universität Wien, Boltzmanngasse 5, 1090 Wien (Austria)
  • 3. Departamento de Química y Física Teóricas, Instituto de Estructura de la Materia (CSIC),Serrano 121, 28006 Madrid (Spain)
  • 4. Departamento de Física Teórica II, Facultad de Ciencias Fśicas,Universidad Complutense de Madrid, Ciudad Universitaria,Plaza Ciencias 1, 28040 Madrid (Spain)
  • 5. Departamento de Ciencias y Tecnología, Universidad Europea de Madrid,Calle Tajo s/n, 28670 Villaviciosa de Odón, Madrid (Spain)

Description

When analyzing the perception of Hawking radiation by different observers, the Hawking effect becomes mixed with the Unruh effect. The separation of both effects is not always clear in the literature. Here we propose an inconsistency-free interpretation of what constitutes a Hawking effect and what an Unruh effect. An appropriate interpretation is important in order to elucidate what sort of effects a detector might experience depending on its trajectory and the state of the quantum field. Under simplifying assumptions we introduce an analytic formula that separates these two effects. Armed with the previous interpretation we argue that for a free-falling detector to cross the horizon without experiencing high-energy effects, it is necessary that the horizon crossing is not attempted at low velocities.

Availability note (English)

Available from http://dx.doi.org/10.1007/JHEP10(2016)161; Available from http://repo.scoap3.org/record/17754

Additional details

Publishing Information

Journal Title
Journal of High Energy Physics (Online)
Journal Volume
2016
Journal Issue
10
Journal Page Range
p. 161
ISSN
1029-8479

INIS

Country of Publication
Germany
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
48059339
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
BLACK HOLES; CONFORMAL INVARIANCE; QUANTUM FIELD THEORY
Descriptors DEC
FIELD THEORIES; INVARIANCE PRINCIPLES

Optional Information

Copyright
Copyright (c) OPEN ACCESS, © The Authors
Notes
PUBLISHER-ID: JHEP10(2016)161; ARXIV:1608.02532; OAI: oai:repo.scoap3.org:17754
Funding organization
SCOAP3, CERN, Geneva (Switzerland)