Transplanckian radiation in theories with extra dimensions
D.V. Gal'tsov

TL;DR
This paper investigates whether particles in high-energy collisions within TeV-scale gravity models can lose all their energy through bremsstrahlung when impact parameters are larger than the black hole's gravitational radius.
Contribution
It analyzes the energy depletion via bremsstrahlung in transplanckian collisions, providing insights into energy loss mechanisms in theories with extra dimensions.
Findings
Particles can significantly lose energy through bremsstrahlung at large impact parameters.
Energy depletion depends on impact parameter and gravitational radius.
Implications for black hole formation in TeV-scale gravity scenarios.
Abstract
We discuss whether the particles undergoing transplanckian collisions in TeV-scale gravity can deplete all their energy on bremsstrahlung for the impact parameters much larger than the gravitational radius of the presumably created black hole.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Pulsars and Gravitational Waves Research
