CMB Distortions from Superconducting Cosmic Strings
arXiv:1202.2474 · doi:10.1103/PhysRevD.85.103522
Abstract
We reconsider the effect of electromagnetic radiation from superconducting strings on cosmic microwave background (CMB) mu- and y-distortions and derive present (COBE-FIRAS) and future (PIXIE) constraints on the string tension, mu_s, and electric current, I. We show that absence of distortions of the CMB in PIXIE will impose strong constraints on mu_s and I, leaving the possibility of light strings (G mu_s < 10^{-18}) or relatively weak currents (I < 10 TeV).
10pages, 5 figures, Submitted to PRD, v2:References added, replaced to match the PRD version
References in corpus (10)
- Cosmic string loop distribution on all length scales and at any redshift
- Cosmic string loops in the expanding universe
- Cosmic Sparks from Superconducting Strings
- Cosmic String Structure at the Gravitational Radiation Scale
- Cosmic String Loops, Large and Small
- Does Bose-Einstein condensation of CMB photons cancel μ distortions created by dissipation of sound waves in the early Universe?
- Constraints on Primordial Black Holes by Distortions of Cosmic Microwave Background
- Radio bursts from superconducting strings
- Scaling solution for small cosmic string loops
- Towards a kinetic theory of strings
Cited by in corpus (35)
- Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum
- PRISM (Polarized Radiation Imaging and Spectroscopy Mission): An Extended White Paper
- Beyond the Standard Models with Cosmic Strings
- Teasing bits of information out of the CMB energy spectrum
- Beyond y and μ: the shape of the CMB spectral distortions in the intermediate epoch, 1.5x10^4 < z < 2x10^5
- Distinguishing different scenarios of early energy release with spectral distortions of the cosmic microwave background
- Green's function of the cosmological thermalization problem
- CMB spectral distortions from small-scale isocurvature fluctuations
- Prospects for Measuring Cosmic Microwave Background Spectral Distortions in the Presence of Foregrounds
- Green's function of the cosmological thermalization problem II: effect of photon injection and constraints
- Observational Constraints on Gauge Field Production in Axion Inflation
- Unavoidable CMB spectral features and blackbody photosphere of our Universe
- A Hydrodynamical Approach to CMB mu-distortions
- Radio Broadcasts from Superconducting Strings
- Constraints on Superconducting Cosmic Strings from the Global -cm Signal before Reionization
- Evolution of CMB spectral distortion anisotropies and tests of primordial non-Gaussianity
- Polarized anisotropic spectral distortions of the CMB: Galactic and extragalactic constraints on photon-axion conversion
- One to rule them all: CMB spectral distortions can probe domain walls, cosmic strings and low scale phase transitions
- Superconducting cosmic strings as sources of cosmological fast radio bursts
- Cosmic Strings in Hidden Sectors: 2. Cosmological and Astrophysical Signatures
- CMB distortion anisotropies due to the decay of primordial magnetic fields
- Cosmological and astrophysical constraints on superconducting cosmic strings
- Constraints on Superconducting Cosmic Strings from Early Reionization
- CMB Distortions from Damping of Acoustic Waves Produced by Cosmic Strings
- A Boltzmann treatment for the vorton excess problem
- CMB Spectral Distortion Constraints on Thermal Inflation
- Updated constraints on superconducting cosmic strings from the astronomy of fast radio bursts
- The Distortion of the Cosmic Microwave Background Spectrum Due to Intergalactic Dust
- CMB Spectral -Distortion of Multiple Inflation Scenario
- Gravitational waves from cosmic strings for pedestrians
- Cosmic Microwave Background Spectral Distortions from Cosmic String Loops
- Test of the Einstein equivalence principle with spectral distortions in the cosmic microwave background
- Topological invariants for superconducting cosmic strings
- Gravitational Scattering Of Photons Off Cosmic Strings
- Constraining self-interacting ultrahigh-energy muon neutrinos by cosmic microwave background spectral distortion