Pith. sign in

REVIEW 2 cited by

Radiation from Atoms Falling into a Black Hole

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1709.00481 v2 pith:FIW7CB2I submitted 2017-09-01 quant-ph gr-qchep-phhep-th

Radiation from Atoms Falling into a Black Hole

classification quant-ph gr-qchep-phhep-th
keywords radiationentropyaccelerationatomsblackfallinghawkinghole
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

We show that atoms falling from outside through a cavity into a black hole (BH) emit acceleration radiation which to a distant observer looks much like Hawking BH radiation. In particular, we find the entropy of the acceleration radiation via a simple laser-like analysis. We call this entropy Horizon Brightened Acceleration Radiation (HBAR) entropy to distinguish it from the BH entropy of Bekenstein and Hawking.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Horizon brightened acceleration radiation from massive vector fields

    gr-qc 2025-12 unverdicted novelty 7.0

    Acceleration radiation for massive vector fields near black hole horizons has a universal thermal detailed-balance factor from the Rindler transformation, with mass thresholds and polarization-dependent spectra, yield...

  2. Ringdown modulation of acceleration radiation in the Schwarzschild background

    gr-qc 2025-11 reject novelty 5.0

    Near a Schwarzschild horizon, a quadrupolar quasinormal ringdown is claimed to modulate the detector detailed-balance exponent by a decaying sinusoid at the QNM frequency, at first order in the perturbation amplitude.