Optical activity of relic neutrino-antineutrino gas
V.B. Semikoz

TL;DR
This paper investigates the optical activity caused by relic neutrino-antineutrino gas in the universe, focusing on the birefringence of electromagnetic waves due to parity violation within the Standard Model, and discusses recent theoretical advances and technical challenges.
Contribution
It revises the problem of electromagnetic birefringence in a chiral medium within the Standard Model, incorporating recent weak correction calculations to improve astrophysical estimates.
Findings
Enhanced understanding of neutrino-induced optical activity
Identification of technical limitations in current measurement methods
Potential implications for astrophysical observations
Abstract
We revise a problem of the birefringence of electromagnetic waves in a chiral medium in the Standard Model (SM) of particle physics arising in an isotropic plasma due to parity violation. The recent calculations of the weak correction to the photon polarization operator in electroweak plasma allow significantly to improve some previous estimates of such effect in astrophysics. Nevertheless, it has remained beyond the abilities of the present technics yet.
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
TopicsDark Matter and Cosmic Phenomena · Cosmology and Gravitation Theories · Neutrino Physics Research
