DOE PAGES title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Pre-Hawking radiation cannot prevent the formation of apparent horizon

Journal Article · · Physical Review D
 [1];  [2];  [3];  [4]
  1. National Taiwan Univ., Taipei (Taiwan). Leung Center for Cosmology and Particle Astrophysics; National Taiwan Univ., Taipei (Taiwan). Dept. of Physics; SLAC National Accelerator Lab., Menlo Park, CA (United States); Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology
  2. Univ. of British Columbia, Vancouver, BC (Canada). Dept. of Physics and Astronomy
  3. National Taiwan Univ., Taipei (Taiwan). Leung Center for Cosmology and Particle Astrophysics; National Taiwan Univ., Taipei (Taiwan). Dept. of Physics; SLAC National Accelerator Lab., Menlo Park, CA (United States)
  4. National Taiwan Univ., Taipei (Taiwan). Leung Center for Cosmology and Particle Astrophysics; Asia Pacific Center for Theoretical Physics, Pohang (Republic of Korea); Postech, Pohan (Republic of Korea). Dept. of Physics

As an attempt to solve the black hole information loss paradox, recently there has been the suggestion that, due to semiclassical effects, a pre-Hawking radiation must exist during the gravitational collapse of matter, which in turn prevents the apparent horizon from forming. Assuming the pre-Hawking radiation does exist, here we argue the opposite. First we note that the stress energy tensor near the horizon for the pre-Hawking radiation is far too small to do anything to the motion of a collapsing shell. Thus the shell will always cross the apparent horizon within a finite proper time. Moreover, the amount of energy that can be radiated must be less than half of the total initial energy (if the particle starts at rest at infinity) before the shell becomes a null shell and cannot radiate any more without becoming tachyonic. Here, we conclude that for any gravitational collapsing process within Einstein gravity and semiclassical quantum field theory, the formation of the apparent horizon is inevitable. Pre-Hawking radiation is therefore not a valid solution to the information paradox.

Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Organization:
Ministry of Science and Technology (MOST); National Taiwan University; Natural Sciences and Engineering Research Council of Canada (NSERC); USDOE
Grant/Contract Number:
AC02-76SF00515; AC03-76SF00515
OSTI ID:
1436413
Journal Information:
Physical Review D, Journal Name: Physical Review D Journal Issue: 6 Vol. 97; ISSN PRVDAQ; ISSN 2470-0010
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English

References (19)

The gravitational field of a radiating star journal May 1951
Comment on self-consistent model of black hole formation and evaporation journal August 2015
The absence of horizon in black-hole formation journal August 2016
The Gravitational Field of a Radiating Star journal January 1999
Vaidya's Radiating Schwarzschild Metric journal March 1965
Energy-momentum tensor near an evaporating black hole journal May 1976
Vacuum polarization in Schwarzschild spacetime journal April 1980
Radiation from collapsing shells, semiclassical backreaction, and black hole formation journal August 2009
Minimal conditions for the existence of a Hawking-like flux journal February 2011
Interior of black holes and information recovery journal February 2016
Model for quantum effects in stellar collapse journal January 2018
Hawking-Like Radiation Does Not Require a Trapped Region journal October 2006
Stress Tensor Calculations and Conformal Anomalies journal December 1977
A Self-Consistent Model of the Black hole Evaporation journal May 2013
Do event horizons exist? journal October 2017
Do event horizons exist? journal October 2017
Radiation from collapsing shells, semiclassical backreaction and black hole formation text January 2009
A Self-consistent Model of the Black Hole Evaporation text January 2013
Model for Quantum Effects in Stellar Collapse text January 2017

Cited By (12)

Information preservation for null shell collapse: a moving mirror model journal July 2019
Testing the nature of dark compact objects: a status report journal July 2019
Role of evaporation in gravitational collapse journal August 2018
Effective black-to-white hole bounces: the cost of surgery journal October 2018
Black hole evaporation and semiclassical thin shell collapse journal September 2019
Understanding black hole evaporation using explicitly computed Penrose diagrams journal January 2020
Phenomenological aspects of black holes beyond general relativity journal December 2018
Charged and Non-Charged Black Hole Solutions in Mimetic Gravitational Theory journal November 2018
Effective black-to-white hole bounces: The cost of surgery text January 2018
Black hole evaporation and semiclassical thin shell collapse text January 2018
Testing the nature of dark compact objects: a status report text January 2019
Understanding black hole evaporation using explicitly computed Penrose diagrams text January 2019

Similar Records

Reflection and transmission at the apparent horizon during gravitational collapse
Journal Article · 2010 · Physical Review. D, Particles Fields · OSTI ID:21432388

Hawking radiation and the boomerang behavior of massive modes near a horizon
Journal Article · 2011 · Physical Review. D, Particles Fields · OSTI ID:21502599

Origin of Hawking radiation
Journal Article · 1987 · Phys. Rev. D; (United States) · OSTI ID:6270513