Extreme electron acceleration with fixed radiation energy
arXiv:2211.00264 · doi:10.3390/e24111570
Abstract
We examine the extreme situation of radiation from an electron that is asymptotically accelerated to the speed of light, resulting in finite emission energy. The analytic solution explicitly demonstrates the difference between radiation power loss and kinetic power loss (null).
arXiv comment8 pages, 8 figures
References in corpus (18)
- New cosmological constraints on primordial black holes
- Time Dependence of Particle Creation from Accelerating Mirrors
- Unruh Effect under Non-equilibrium conditions: Oscillatory motion of an Unruh-DeWitt detector
- Effects of Horizons on Entanglement Harvesting
- The symmetry, inferable from Bogoliubov transformation, between the processes induced by the mirror in two-dimentional and the charge in four-dimentional space-time
- Reflecting at the Speed of Light
- Quantum power distribution of relativistic acceleration radiation: classical electrodynamic analogies with perfectly reflecting moving mirrors
- Compatibility of Larmor's formula with radiation reaction for a radiating charge
- Radiation from an inertial mirror horizon
- Infrared acceleration radiation
- Relativistic quantum information as radiation reaction: entanglement entropy and self-force of a moving mirror analog to the CGHS black hole
- Möbius Mirrors
- Light and Airy: a simple solution for relativistic quantum acceleration radiation
- Quantum power: a Lorentz invariant approach to Hawking radiation
- Radiation from Comoving Poynting Flux Acceleration
- Disparities of Larmor's/Liénard's formulations with special relativity and energy-momentum conservation
- Stationary Worldline Power Distributions
- Discrepancy between power radiated and the power loss due to radiation reaction for an accelerated charge
Cited by in corpus (7)
- Infrared acceleration radiation
- Accelerated electron thermometer: observation of 1D Planck radiation
- Electron as a Tiny Mirror: Radiation From a Worldline With Asymptotic Inertia
- Thermal Larmor radiation
- IR-finite thermal acceleration radiation
- Stopping to Reflect: Asymptotic Static Moving Mirrors as Quantum Analogs of Classical Radiation
- Classical acceleration temperature from evaporated black hole remnants and accelerated electron-mirror radiation