Built on

M. A. Fedderke, P. W. Graham, and S. Rajendran, Axion Dark Matter Detection with CMB Polarization, Phys. Rev. D 100
Original
1903
Earlier work this paper cites.
Y. Minami, H. Ochi, K. Ichiki, N. Katayama, E. Komatsu, and T. Matsumura, Simultaneous determination of the cosmic birefringence and miscalibrated polarization angles from CMB experiments, PTEP 2019
Original
1904
Earlier work this paper cites.
V. Aragam, S. Paban, and R. Rosati, Multi-field Inflation in High-Slope Potentials, JCAP 04
Original
1905
Earlier work this paper cites.
P. Christodoulidis, D. Roest, and R. Rosati, Many-field Inflation: Universality or Prior Dependence?, JCAP 04
Original
1907
Earlier work this paper cites.
J. Halverson, C. Long, B. Nelson, and G. Salinas, Towards string theory expectations for photon couplings to axionlike particles, Phys. Rev. D 100
Original
1909
Earlier work this paper cites.
D. J. Gross, R. D. Pisarski, and L. G. Yaffe, QCD and Instantons at Finite Temperature, Rev. Mod. Phys. 53
1981
Earlier work this paper cites.
J. Preskill, M. B. Wise, and F. Wilczek, Cosmology of the Invisible Axion, Phys. Lett. B 120
1983
Earlier work this paper cites.
L. F. Abbott and P. Sikivie, A Cosmological Bound on the Invisible Axion, Phys. Lett. B 120
1983
Earlier work this paper cites.
M. Dine and W. Fischler, The Not So Harmless Axion, Phys. Lett. B 120
1983
Earlier work this paper cites.
M. S. Turner, Coherent Scalar Field Oscillations in an Expanding Universe, Phys. Rev. D 28
1983
Earlier work this paper cites.
N. Kaloper and L. Sorbo, A Natural Framework for Chaotic Inflation, Phys. Rev. Lett. 102
Original
1989
Earlier work this paper cites.
S. M. Carroll, G. B. Field, and R. Jackiw, Limits on a Lorentz and Parity Violating Modification of Electrodynamics, Phys. Rev. D 41
1990
Earlier work this paper cites.
E. W. Kolb and M. S. Turner, The Early Universe , Vol. 69 (1990)
1990
Earlier work this paper cites.
S. M. Carroll and G. B. Field, Einstein equivalence principle and the polarization of radio galaxies, Phys. Rev. D 43
1991
Earlier work this paper cites.
D. Harari and P. Sikivie, Effects of a Nambu-Goldstone boson on the polarization of radio galaxies and the cosmic microwave background, Phys. Lett. B 289
1992
Earlier work this paper cites.
A. Sklar, Random variables, distribution functions, and copulas: A personal look backward and forward, Lecture Notes-Monograph Series 28
1996
Earlier work this paper cites.
A. Lue, L.-M. Wang, and M. Kamionkowski, Cosmological signature of new parity violating interactions, Phys. Rev. Lett. 83
1999
Earlier work this paper cites.
T. Namikawa et al. , Atacama Cosmology Telescope: Constraints on cosmic birefringence, Phys. Rev. D 101
Original
2001
Earlier work this paper cites.
Y. Minami and E. Komatsu, Simultaneous determination of the cosmic birefringence and miscalibrated polarization angles II: Including cross frequency spectra, PTEP 2020
Original
2006
Earlier work this paper cites.
F. Bianchini et al. (SPT), Searching for Anisotropic Cosmic Birefringence with Polarization Data from SPTpol, Phys. Rev. D 102
Original
2006
Earlier work this paper cites.
H. Zhai, S.-Y. Li, M. Li, H. Li, and X. Zhang, The effects on CMB power spectra and bispectra from the polarization rotation and its correlations with temperature and E-polarization, JCAP 12
Original
2006
Earlier work this paper cites.
T. Fujita, Y. Minami, K. Murai, and H. Nakatsuka, Probing axionlike particles via cosmic microwave background polarization, Phys. Rev. D 103
Original
2008
Earlier work this paper cites.
E. Silverstein and A. Westphal, Monodromy in the CMB: Gravity Waves and String Inflation, Phys. Rev. D 78
Original
2008
Earlier work this paper cites.

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Original
2009
Cited alongside, same era.
F. Finelli and M. Galaverni, Rotation of Linear Polarization Plane and Circular Polarization from Cosmological Pseudo-Scalar Fields, Phys. Rev. D 79
Original
2009
Cited alongside, same era.
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Original
2010
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Original
2010

Then

G. Sigl and P. Trivedi, Axion-like Dark Matter Constraints from CMB Birefringence, (2018), arXiv:1811.07873 [astro-ph.CO]
Original
2018
Later among the works it cites.
T. C. Bachlechner, K. Eckerle, O. Janssen, and M. Kleban, Multiple-axion framework, Phys. Rev. D 98
Original
2018
Later among the works it cites.
J. Alvey and M. Escudero Abenza, Constraints on global symmetry breaking in quantum gravity from cosmic birefringence measurements, Phys. Lett. B 823
Original
2021
Later among the works it cites.
B. D. Sherwin and T. Namikawa, Cosmic birefringence tomography and calibration-independence with reionization signals in the CMB, (2021), arXiv:2108.09287 [astro-ph.CO]
Original
2021
Later among the works it cites.
G. D’Amico, N. Kaloper, and A. Westphal, Double Monodromy Inflation: A Gravity Waves Factory for CMB-S4, LiteBIRD and LISA, Phys. Rev. D 104

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2023

Cosmic Birefringence from the Axiverse

Gasparotto, Silvia, Sfakianakis, Evangelos I.

Understand

We revisit the evidence for CMB birefringence in the context of a rich Axiverse.

Using probability density functions (PDFs) for various axion parameters, such as the mass and axion decay constant, we construct the PDF for the cosmic birefringence angle and investigate its properties.
By relating the observed value of the birefringence angle to the mean or standard deviation of the constructed PDF, we constrain the shape of the input PDFs, providing insights into the statistical distribution of the Axiverse.
We focus on three different types of axion potentials: cosine, quadratic, and asymptotically linear axion monodromy.