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Final burst of the moving mirror is unrelated to the partner mode of analog Hawking radiation

Journal Article · · Physical Review. D.
 [1];  [2];  [3];  [4];  [5]
  1. Nagoya Univ. (Japan); SLAC
  2. National Taiwan Univ., Taipei (Taiwan)
  3. Nagoya Univ. (Japan)
  4. Tohoku Univ., Sendai (Japan); National Taiwan Univ., Taipei (Taiwan)
  5. National Taiwan Univ., Taipei (Taiwan); Stanford Univ., CA (United States). Kavli Institute for Particle Astrophysics & Cosmology; SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Flying mirrors with appropriate trajectories have been recognized as an analog system that mimics black hole Hawking evaporation and have been widely investigated. It has recently been suggested that the partner mode of the analog Hawking radiation emitted from a moving mirror would manifest itself through a final burst when the mirror executes a sudden stop. Here, in this study, we argue the opposite via the partner formula for the moving mirror model. By expanding the theoretical foundation of the partner formula and augmenting it with numerical analysis, we demonstrate that the supposed final burst is induced by a shock that requires the input of external energy, whereas the Hawking radiation partner mode, which is associated with the zero-point vacuum fluctuations, is not responsible for the burst.
Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Organization:
Japan Science and Technology Agency (JST); Japan Society for the Promotion of Science (JSPS); Ministry of Education, Culture, Sports, Science and Technology (MEXT); Nagoya University; USDOE Office of Science (SC)
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
2447163
Journal Information:
Physical Review. D., Journal Name: Physical Review. D. Journal Issue: 2 Vol. 110; ISSN 2470-0010
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English

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