Download presentation
Presentation is loading. Please wait.
Published byMarybeth Chapman Modified over 9 years ago
1
CMB constraints on Lorentz violation in the neutrino sector Zong-Kuan Guo (ITP, CAS) Weihai August 13, 2012
2
outline motivations deformed dispersion relation Boltzmann equation cosmological constraints remarks This talk is based on ZKG, Q-G Huang, R-G Cai, Y-Z Zhang, PRD in press [arXiv:1206.5588]
3
motivations neutrino oscillations neutrinos influence the CMB (massive or massless) neutrinos influence the LSS
4
the deformed dispersion relation the scalar perturbations of the FLRW metric in the synchronous gauge
5
the action in the first-order formalism the Lagrangian in the synchronous gauge
6
the number density, energy density and pressure the perturbed energy density, pressure, energy flux and shear stress
7
the Boltzmann equation
8
the initial conditions
10
cosmological constraints
11
remarks Compared to particle physics experiments, cosmological observations yield much weaker constraints on the Lorentz-violation parameter in the neutrino sector. We neglects neutrino oscillations, possible species dependence, anisotropies associated with violations of rotation symmetry, and CPT violation.
12
Thanks!
Similar presentations
© 2025 SlidePlayer.com. Inc.
All rights reserved.