Isotropic cosmic birefringence from early dark energy - INSPIRE

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Isotropic cosmic birefringence from early dark energy

Kai Murai
(
- Tokyo U., ICRR and
- Tokyo U., IPMU
)
,
Fumihiro Naokawa
(
- Tokyo U. and
- Tokyo U., RESCEU
)
,
Toshiya Namikawa
(
- Tokyo U., IPMU
)
,
Eiichiro Komatsu
(
- Tokyo U., IPMU and
- Garching, Max Planck Inst.
)

Sep 16, 2022

7 pages

Published in:

Phys.Rev.D 107 (2023) 4, L041302

Published: Feb 15, 2023

e-Print:

2209.07804 [astro-ph.CO]

DOI:

10.1103/PhysRevD.107.L041302 (publication)

Report number:

RESCEU-16/22

View in:

reference search49 citations

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Abstract: (APS)

A tantalizing hint of isotropic cosmic birefringence has been found in the

E B

cross-power spectrum of the cosmic microwave background (CMB) polarization data with a statistical significance of

3 σ

. A pseudoscalar field coupled to the CMB photons via the Chern-Simons term can explain this observation. The same field may also be responsible for early dark energy (EDE), which alleviates the so-called Hubble tension. Since the EDE field evolves significantly during the recombination epoch, the conventional formula that relates

E B

to the difference between the

E

- and

B

-mode autopower spectra is no longer valid. Solving the Boltzmann equation for polarized photons and the dynamics of the EDE field consistently, we find that currently favored parameter space of the EDE model yields a variety of shapes of the

E B

spectrum, which can be tested by CMB experiments.

Note:

7 pages, 4 figures, 1 table. (v2) Expanded discussion on forecasts for SO and CMB-S4. Accepted for publication in Phys. Rev. D

cosmic background radiation: spectrum
birefringence
photon: coupling
dark energy
tension
recombination
polarization
Chern-Simons term
statistical analysis: confidence limit
Boltzmann equation

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