The global 21-cm signal of a network of cosmic string wakes
Abstract
In previous works, we discussed the 21-cm signature of a single cosmic string wake. However, the 21-cm brightness temperature is influenced by a network of cosmic string wakes, and not one single wake. In this work, we consider the signal from a network of wakes laid down during the matter era. We also improve on the previous calculation of a single wake signature. Finally, we calculate the enhancement of the global 21-cm brightness temperature due to a network of wakes and discuss its affects of the signal measured in the Wouthuysen-Field absorption trough. We estimated that for string tensions between 10-8 and 10-7 there would be between a 10 per cent and a factor of 2 enhancement in the signal.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- November 2021
- DOI:
- 10.1093/mnras/stab2634
- arXiv:
- arXiv:2108.08220
- Bibcode:
- 2021MNRAS.508..408H
- Keywords:
-
- intergalactic medium;
- cosmic background radiation;
- dark ages;
- reionization;
- first stars;
- diffuse radiation;
- cosmology: theory;
- Astrophysics - Cosmology and Nongalactic Astrophysics;
- High Energy Physics - Phenomenology;
- High Energy Physics - Theory
- E-Print:
- 6 pages, 4 figure. v2 to v3: minor typo corrected in references. v1 to v2: explanation in section 5 expanded, figures enlarged, NANOGrav data description changed in section 2, 1 references added in section 2. Matches the version accepted for publication by MNRAS