Cosmic Rays and Spectral Distortions from Collapsing Textures

TL;DR

This paper analyzes the photon and neutrino spectra produced by cosmic textures, exploring their impact on high-energy cosmic rays and CMB spectral distortions, and discusses constraints from current and future observations.

Contribution

It provides detailed calculations of photon and neutrino spectra from cosmic textures and evaluates their implications for cosmic ray and CMB spectral distortion constraints.

Findings

Textures contribute to high-energy photon flux with a specific energy dependence.

Current COBE bounds are weaker than CMB angular power spectrum constraints.

Future surveys like PIXIE can impose stronger limits on texture models.

Abstract

We compute the energy spectrum of photons and neutrinos produced by the unwinding of a scaling distribution of cosmic textures, and discuss the implications for the spectrum of high energy cosmic rays, and for CMB spectral distortions. Textures lead to a contribution to the photon flux which scales as $E^3 F(E) \sim E^{3/2}$. Hence, the tightest constraints on the texture model come from the highest energies from which primordial photons can reach us without being scattered by the CMB and other foregrounds. Textures lead to both $\mu$ type and $y$ type distortions. While the constraints on the texture model coming from the current COBE bounds are weaker than the bounds from the angular power spectrum of the CMB, future surveys such as PIXIE can lead to stronger bounds. The high energy neutrino flux is constrained by data from the Pierre Auger experiment and yields a bound on the energy scale of textures which is competitive with CMB bounds.