Parity-violating scalar trispectrum from a rolling axion during inflation
Abstract: We study a mechanism of generating the trispectrum (4-point correlation) of curvature perturbation through the dynamics of a spectator axion field and U(1) gauge field during inflation. Owing to the Chern-Simons coupling, only one helicity mode of gauge field experiences a tachyonic instability and sources scalar perturbations. Sourced curvature perturbation exhibits parity-violating nature which can be tested through its trispectrum. We numerically compute parity-even and parity-odd component of the sourced trispectrum. It is found that the ratio of parity-odd to parity-even mode can reach O(10%) in an exact equilateral momentum configuration. We also investigate a quasi-equilateral shape where only one of the momenta is slightly longer than the other three, and find that the parity-odd mode can reach, and more interestingly, surpass the parity-even one. This may help us to interpret a large parity-odd trispectrum signal extracted from BOSS galaxy-clustering data.
- Y. Minami and E. Komatsu, Phys. Rev. Lett. 125, 221301 (2020), arXiv:2011.11254 [astro-ph.CO] .
- P. Diego-Palazuelos et al., Phys. Rev. Lett. 128, 091302 (2022), arXiv:2201.07682 [astro-ph.CO] .
- J. R. Eskilt, Astron. Astrophys. 662, A10 (2022), arXiv:2201.13347 [astro-ph.CO] .
- J. R. Eskilt and E. Komatsu,  (2022), arXiv:2205.13962 [astro-ph.CO] .
- J. R. Eskilt et al.,  (2023a), arXiv:2305.02268 [astro-ph.CO] .
- S. M. Carroll, Phys. Rev. Lett. 81, 3067 (1998), astro-ph/9806099 .
- I. Obata, JCAP 09, 062 (2022), 2108.02150 .
- S. Gasparotto and I. Obata, JCAP 08, 025 (2022), arXiv:2203.09409 [astro-ph.CO] .
- S. Gasparotto and E. I. Sfakianakis,  (2023), arXiv:2306.16355 [astro-ph.CO] .
- F. Finelli and M. Galaverni, Phys. Rev. D 79, 063002 (2009), 0802.4210 .
- G.-C. Liu and K.-W. Ng, Phys. Dark Univ. 16, 22 (2017), 1612.02104 .
- F. Takahashi and W. Yin, JCAP 04, 007 (2021), arXiv:2012.11576 [hep-ph] .
- P. A. R. Ade et al. (Planck), Astron. Astrophys. 594, A17 (2016), arXiv:1502.01592 [astro-ph.CO] .
- Y. Akrami et al. (Planck), Astron. Astrophys. 641, A9 (2020), arXiv:1905.05697 [astro-ph.CO] .
- L. Sorbo, JCAP 1106, 003 (2011), arXiv:1101.1525 [astro-ph.CO] .
- J. L. Cook and L. Sorbo, Phys. Rev. D85, 023534 (2012), [Erratum: Phys. Rev.D86,069901(2012)], arXiv:1109.0022 [astro-ph.CO] .
- J. L. Cook and L. Sorbo, JCAP 1311, 047 (2013), arXiv:1307.7077 [astro-ph.CO] .
- I. Obata, JCAP 06, 050 (2017), arXiv:1612.08817 [astro-ph.CO] .
- O. Özsoy, JCAP 04, 040 (2021), arXiv:2005.10280 [astro-ph.CO] .
- X. Niu and M. H. Rahat,  (2023), arXiv:2307.01192 [hep-ph] .
- A. Maleknejad and M. Sheikh-Jabbari, Phys. Rev. D 84, 043515 (2011), arXiv:1102.1932 [hep-ph] .
- E. Dimastrogiovanni and M. Peloso, Phys. Rev. D 87, 103501 (2013), arXiv:1212.5184 [astro-ph.CO] .
- P. Adshead and E. I. Sfakianakis, JHEP 08, 130 (2017), arXiv:1705.03024 [hep-th] .
- E. Komatsu, Nature Rev. Phys. 4, 452 (2022), arXiv:2202.13919 [astro-ph.CO] .
- M. Shiraishi, Phys. Rev. D 94, 083503 (2016), arXiv:1608.00368 [astro-ph.CO] .
- O. H. E. Philcox, Phys. Rev. D 106, 063501 (2022), arXiv:2206.04227 [astro-ph.CO] .
- O. H. E. Philcox,  (2023), arXiv:2303.12106 [astro-ph.CO] .
- O. H. E. Philcox and M. Shiraishi,  (2023), arXiv:2308.03831 [astro-ph.CO] .
- M. Shiraishi, JCAP 06, 015 (2012), arXiv:1202.2847 [astro-ph.CO] .
Paper Prompts
Sign up for free to create and run prompts on this paper using GPT-5.
Top Community Prompts
Collections
Sign up for free to add this paper to one or more collections.