activity
20242026
most citedClassical acceleration temperature from evaporated black hole remnants and accelerated electron-mirror radiation

4 citations · 10 across the 12 of their papers we have counts for

collaborators

12 papers

gr-qc2026

Squeezed quantum states and partner modes in the moving mirror model of black hole evaporation

Kuan-Nan Lin, Pisin Chen, Michael R. R. Good +1

The standard moving mirror model in (1+1)-dimensional spacetime is known to reproduce several quantum aspects of black hole evaporation. A perfectly reflecting, accelerating mirror…

gr-qc2026

Optical and thermodynamic properties of Kerr-Bertotti-Robinson black holes

Hassan Hassanabadi, Michael R. R. Good, Soroush Zare +2

We investigate the thermodynamic and optical properties of Kerr--Bertotti--Robinson black holes, namely rotating black holes immersed in an external Bertotti--Robinson electromagne…

physics.class-ph2026

An advanced undergraduate derivation of acceleration thermality

Michael R. R. Good

The thermal radioactivity of beta-decay photons, described by a 1D Planck distribution, can be modeled as classical radiation emitted by an accelerated electron. Here, we present t…

gr-qc2026

Frenet-Serret equations with variable proper acceleration in Minkowski spacetime

Ivan Perez-Roman, Michael R. R. Good, Yen Chin Ong +1

We study Frenet-Serret equations for timelike worldlines in Minkowski spacetime with proper-time-dependent curvature and torsion. This corresponds to relativistic motion with non-u…

quant-ph2026

Apparent Fermionic Spectra for Bosonic Radiation: Accelerated Charge Kinematics

Michael R. R. Good, Evgenii Ievlev, Arsen Almaskhan

An accelerated point charge can emit photons with an apparent Fermi-Dirac spectrum, even though the radiation is bosonic and its occupation numbers are not constrained to 0 or 1. T…

gr-qc2026

Planckian Gravitons from an Imaginary-Time Clock

Michael R. R. Good, Eric V. Linder

We present a simple derivation of the exact Planck spectrum of the quadrupole radiation from point masses moving apart nonrelativistically, essentially an analog for gravitational…

gr-qc2026

Self-Reflection in a Moving Mirror

Michael R. R. Good, Eric V. Linder

We present an analytic flat-spacetime accelerating boundary analog of Hawking-type emission that possesses infinite asymptotic acceleration (and radial acceleration in the black ho…

quant-ph2025

Particle creation from entanglement entropy

Michael R. R. Good, Evgenii Ievlev, Eric V. Linder

We investigate how entanglement entropy can drive particle creation, deriving explicit relations between entropy and the radiated particle spectrum, the total number of particles,…

gr-qc2024★ 2 cited

Hawking Temperature and the Inverse-Radius Scale of the Horizon

Michael R. R. Good, Yen Chin Ong

The Hawking temperature of a Schwarzschild black hole can be heuristically derived by identifying the temperature with the inverse radius of the horizon up to a multiplicative cons…

quant-ph2024★ 3 cited

Electron-mirror duality and thermality

Evgenii Ievlev, Michael R. R. Good, Paul C. W. Davies

Classical electromagnetic radiation from moving point charges is foundational, but the thermal dynamics responsible for classical acceleration temperature are poorly understood. We…

physics.class-ph2024★ 1 cited

Classical Acceleration Temperature (CAT) in a Box

Ahsan Mujtaba, Maksat Temirkhan, Yen Chin Ong +1

A confined, slow-moving, accelerating electron is shown to emit thermal radiation. Since laboratories face spatial constraints when dealing with rectilinear motion, focusing on a f…

gr-qc2024★ 4 cited

Classical acceleration temperature from evaporated black hole remnants and accelerated electron-mirror radiation

Kuan-Nan Lin, Evgenii Ievlev, Michael R. R. Good +1

We investigate the radiation from accelerating electrons with asymptotic constant velocity and their analog signatures as evaporating black holes with left-over remnants. We find h…