Future CMB constraints on cosmic birefringence and implications for fundamental physics
arXiv:1904.07855 · doi:10.1103/PhysRevD.100.023507
Abstract
The primary scientific target of the CMB polarization experiments that are currently being built and proposed is the detection of primordial tensor perturbations. As a byproduct, these instruments will significantly improve constraints on cosmic birefringence, or the rotation of the CMB polarization plane. If convincingly detected, cosmic birefringence would be a dramatic manifestation of physics beyond the standard models of particle physics and cosmology. We forecast the bounds on the cosmic polarization rotation (CPR) from the upcoming ground-based Simons Observatory (SO) and the space-based LiteBIRD experiments, as well as a "fourth generation" ground-based CMB experiment like CMB-S4 and the mid-cost space mission PICO. We examine the detectability of both a stochastic anisotropic rotation field and an isotropic rotation by a constant angle. CPR induces new correlations of CMB observables, including spectra of parity-odd type in the case of isotropic CPR, and mode-coupling correlations in the anisotropic rotation case. We find that LiteBIRD and SO will reduce the 1 bound on the isotropic CPR from the current value of 30 arcmin to 1.5 and 0.6 arcmin, respectively, while CMB-S4-like and PICO will reduce it to arcmin. The bounds on the amplitude of a scale-invariant CPR spectrum will be reduced by 1, 2 and 3 orders of magnitude by LiteBIRD, SO and CMB-S4-like/PICO, respectively. We discuss implications of the forecasted CPR bounds for pseudoscalar fields, primordial magnetic fields (PMF), and violations of Lorentz invariance. We find that CMB-S4-like and PICO can reduce the 1 bound on the amplitude of the scale-invariant PMF from 1 nG to 0.1 nG, while also probing the magnetic field of the Milky Way. They will also significantly improve bounds on the axion-photon coupling, placing stringent constraints on the string theory axions.
14 pages, 1 figure, 5 tables; minor corrections in V2, matches the version published in PRD
References in corpus (38)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Cosmology and the Fate of Dilatation Symmetry
- A Joint Analysis of BICEP2/Keck Array and Planck Data
- Electrodynamics with Lorentz-violating operators of arbitrary dimension
- Lower limit on the strength and filling factor of extragalactic magnetic fields
- What Do We Know About Lorentz Invariance?
- Sensitive polarimetric search for relativity violations in gamma-ray bursts
- Lorentz-violating electrodynamics and the cosmic microwave background
- Cosmic Microwave Background Statistics for a Direction-Dependent Primordial Power Spectrum
- CMB anisotropies from primordial inhomogeneous magnetic fields
- Parity violation constraints using 2006-2007 QUaD CMB polarization spectra
- Measurements of Sub-degree B-mode Polarization in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data
- Effect on cosmic microwave background polarization of coupling of quintessence to pseudoscalar formed from the electromagnetic field and its dual
- Magnetic field production during preheating at the electroweak scale
- CMB Polarization Systematics Due to Beam Asymmetry: Impact on Inflationary Science
- Self-Calibration of CMB Polarization Experiments
- Pseudoscalar perturbations and polarization of the cosmic microwave background
- How to De-Rotate the Cosmic Microwave Background Polarization
- New CMB constraints for Abelian Higgs cosmic strings
- De-Rotation of the Cosmic Microwave Background Polarization: Full-Sky Formalism
- Constraints on CPT violation from WMAP three year polarization data: a wavelet analysis
- The Impact of Stochastic Primordial Magnetic Fields on the Scalar Contribution to Cosmic Microwave Background Anisotropies
- Faraday Rotation Limits on a Primordial Magnetic Field from WMAP Five-Year Data
- Measuring the speed of cosmological gravitational waves
- CMB Polarization Systematics, Cosmological Birefringence and the Gravitational Waves Background
- Effects of modified gravity on B-mode polarization
- Constraining a spatially dependent rotation of the Cosmic Microwave Background Polarization
- How to simulate global cosmic strings with large string tension
- Constraints on Primordial Magnetic Fields from Planck combined with the South Pole Telescope CMB B-mode polarization measurements
- Testing CPT Symmetry with CMB Measurements
- Testing Lorentz Invariance Violation with WMAP Five Year Data
- PICO: Probe of Inflation and Cosmic Origins
- Fluctuations of cosmological birefringence and the effect on CMB B-mode polarization
- Confronting pNGB quintessence with data
- Neutrino number asymmetry and cosmological birefringence
- Testing CPT Symmetry with Current and Future CMB Measurements
- Impact of Instrumental Systematic Contamination on the Lensing Mass Reconstruction using the CMB Polarization
- Impact of Instrumental Systematics on the CMB Bispectrum
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- Searching for Anisotropic Cosmic Birefringence with Polarization Data from SPTpol
- Searching for axion-like particles through CMB birefringence from string-wall networks
- Cosmic Birefringence: Cross-Spectra and Cross-Bispectra with CMB Anisotropies
- Simultaneous determination of the cosmic birefringence and miscalibrated polarisation angles from CMB experiments
- Finding Evidence for Inflation and the Origin of Galactic Magnetic Fields with CMB Surveys
- Simultaneous determination of the cosmic birefringence and miscalibrated polarization angles II: Including cross frequency spectra
- Constraining cosmic polarization rotation and implications for primordial B-modes
- Nonminimal Lorentz Violation in Macroscopic Matter