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Abstract
The North American Nanohertz Observatory for Gravitational Waves has recently reported strong evidence for a stochastic common-spectrum process affecting the pulsar timing residuals in its 12.5-year data set. We demonstrate that this process admits an interpretation in terms of a stochastic gravitational-wave background emitted by a cosmic-string network in the early Universe. We study stable Nambu-Goto strings in dependence of their tension Gμ and loop size α and show that the entire viable parameter space will be probed by an array of future experiments.
Original language | English |
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Article number | 041305 |
Number of pages | 7 |
Journal | Phys. Rev. Lett. |
Volume | 126 |
Issue number | 4 |
DOIs | |
Publication status | Published - 28 Jan 2021 |
Bibliographical note
7 pages, 3 figures. v2: revised treatment of the higher cosmic-string modes [see Eq. (6)], resulting in a few numerical but no qualitative changes. v3: matches version published in PRLKeywords
- astro-ph.CO
- gr-qc
- hep-ph
- hep-th
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Dive into the research topics of 'Has NANOGrav found first evidence for cosmic strings?'. Together they form a unique fingerprint.Projects
- 1 Active
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SRP8: Strategic Research Programme: High-Energy Physics at the VUB
D'Hondt, J., Van Eijndhoven, N., Craps, B. & Buitink, S.
1/11/12 → 31/10/24
Project: Fundamental