Relaxing cosmological constraints on current neutrino masses: Acknowledgment, Appendix & References by@cosmological
256 reads
Relaxing cosmological constraints on current neutrino masses: Acknowledgment, Appendix & References
by Cosmological thinking: time, space and universal causation May 24th, 2024
Too Long; Didn't Read
In this paper, researchers present a mass-varying neutrino model driven by scalar field dark energy, relaxing the upper bound on current neutrino mass.
This paper is available on arxiv under CC 4.0 license.
Authors:
(1) Vitor da Fonseca, Instituto de Astrof´ısica e Ciˆencias do Espa¸co, Faculdade de Ciˆencias da Universidade de Lisboa;
(2) Tiago Barreiro, Instituto de Astrof´ısica e Ciˆencias do Espa¸co, Faculdade de Ciˆencias da Universidade de Lisboa and 2ECEO, Universidade Lus´ofona;
(3) Nelson J. Nunes, Instituto de Astrof´ısica e Ciˆencias do Espa¸co, Faculdade de Ciˆencias da Universidade de Lisboa.
Table of Links
- Abstract and Intro
- Coupling Dark Energy to Neutrinos
- Impact of the Coupling on Perturbations and Observables
- Parameter Estimation
- Discussion
- Acknowledgment, Appendix, and References
ACKNOWLEDGMENTS
The authors would like to thank C. van de Bruck and D. F. Mota for the fruitful discussions. This work is supported by the Funda¸c˜ao para a Ciˆencia e a Tecnologia (FCT) through the research grants UIDB/04434/2020 and UIDP/04434/2020, and the BEYLA project PTDC/FIS-AST/0054/2021. V.d.F. acknowledges FCT support through fellowship 2022.14431.BD.
Appendix A: Parameter constraints for the MaVaN and the uncoupled scalar field models
In the appendix we show the triangular plots of the analysis made with the Plk18+BAO data for the MaVaN model (β free) and the uncoupled case (β = 0), i.e. no interaction between the quintessence component and the neutrino fluid.
References
[1] J. Lesgourgues and S. Pastor, Phys. Rept. 429, 307 (2006), arXiv:astro-ph/0603494.
[2] M. Gerbino and M. Lattanzi, Frontiers in Physics 5 (2018), 10.3389/fphy.2017.00070.
[3] Y. Fukuda et al. (Super-Kamiokande), Phys. Rev. Lett. 81, 1562 (1998), arXiv:hep-ex/9807003.
[4] K. Abe et al. (T2K), Phys. Rev. Lett. 112, 061802 (2014), arXiv:1311.4750 [hep-ex].
[5] I. Esteban, M. C. Gonzalez-Garcia, A. HernandezCabezudo, M. Maltoni, and T. Schwetz, JHEP 01, 106 (2019), arXiv:1811.05487 [hep-ph].
[6] S. Roy Choudhury and S. Hannestad, JCAP 07, 037 (2020), arXiv:1907.12598 [astro-ph.CO].
[7] M. Aker et al. (KATRIN), Phys. Rev. Lett. 123, 221802 (2019), arXiv:1909.06048 [hep-ex].
[8] S. S. Gershtein and Y. B. Zel’dovich, ZhETF Pisma Redaktsiiu 4, 174 (1966).
[9] N. Aghanim et al. (Planck), A&A 641, A6 (2020), [Erratum: Astron.Astrophys. 652, C4 (2021)], arXiv:1807.06209 [astro-ph.CO].
[10] R. L. Workman et al. (Particle Data Group), PTEP 2022, 083C01 (2022).
[11] A. G. Riess et al. (Supernova Search Team), Astron. J. 116, 1009 (1998), arXiv:astro-ph/9805201.
[12] S. Perlmutter et al. (Supernova Cosmology Project), Astrophys. J. 517, 565 (1999), arXiv:astroph/9812133.
[13] P. Gu, X. Wang, and X. Zhang, Phys. Rev. D 68, 087301 (2003), arXiv:hep-ph/0307148.
[14] R. Fardon, A. E. Nelson, and N. Weiner, JCAP 10, 005 (2004), arXiv:astro-ph/0309800.
[15] R. D. Peccei, Phys. Rev. D 71, 023527 (2005), arXiv:hep-ph/0411137.
[16] A. W. Brookfield, C. van de Bruck, D. F. Mota, and D. Tocchini-Valentini, Phys. Rev. D 73, 083515 (2006), [Erratum: Phys.Rev.D 76, 049901 (2007)], arXiv:astro-ph/0512367.
[17] C. Wetterich, Phys. Lett. B 655, 201 (2007), arXiv:0706.4427 [hep-ph].
[18] L. Amendola, M. Baldi, and C. Wetterich, Phys. Rev. D 78, 023015 (2008), arXiv:0706.3064 [astro-ph].
[19] K. Ichiki and Y.-Y. Keum, JCAP 06, 005 (2008), arXiv:0705.2134 [astro-ph].
[20] U. Franca, M. Lattanzi, J. Lesgourgues, and S. Pastor, Phys. Rev. D 80, 083506 (2009), arXiv:0908.0534 [astro-ph.CO].
[21] C.-Q. Geng, C.-C. Lee, R. Myrzakulov, M. Sami, and E. N. Saridakis, JCAP 01, 049 (2016), arXiv:1504.08141 [astro-ph.CO].
[22] N. J. Nunes and J. E. Lidsey, Phys. Rev. D 69, 123511 (2004), arXiv:astro-ph/0310882.
[23] P. J. E. Peebles and B. Ratra, apjl 325, L17 (1988).
[24] V. da Fonseca, T. Barreiro, N. J. Nunes, S. Cristiani, et al., Astronomy & Astrophysics (2022), 10.1051/0004-6361/202243795.
[25] B. J. Barros and V. da Fonseca, JCAP 06, 048 (2023), arXiv:2209.12189 [astro-ph.CO].
[26] V. da Fonseca, T. Barreiro, and N. J. Nunes, Phys. Dark Univ. 35, 100940 (2022), arXiv:2104.14889 [astro-ph.CO].
[27] D. F. Mota, V. Pettorino, G. Robbers, and C. Wetterich, Phys. Lett. B 663, 160 (2008), arXiv:0802.1515 [astro-ph].
[28] N. J. Nunes, L. Schrempp, and C. Wetterich, Phys. Rev. D 83, 083523 (2011), arXiv:1102.1664 [astroph.CO].
[29] J. Sakstein and M. Trodden, Phys. Rev. Lett. 124, 161301 (2020), arXiv:1911.11760 [astro-ph.CO].
[30] M. Carrillo Gonz´alez, Q. Liang, J. Sakstein, and M. Trodden, (2023), arXiv:2302.09091 [astro-ph.CO].
[31] A. G. Riess, S. Casertano, W. Yuan, L. M. Macri, and D. Scolnic, Astrophys. J. 876, 85 (2019), arXiv:1903.07603 [astro-ph.CO].
[32] K. C. Wong et al., Mon. Not. Roy. Astron. Soc. 498, 1420 (2020), arXiv:1907.04869 [astro-ph.CO].
[33] A. G. Riess, S. Casertano, W. Yuan, J. B. Bowers, L. Macri, J. C. Zinn, and D. Scolnic, Astrophys. J. Lett. 908, L6 (2021), arXiv:2012.08534 [astro-ph.CO].
[34] J. Lesgourgues, “The cosmic linear anisotropy solving system (class) i: Overview,” (2011), arXiv:1104.2932 [astro-ph.IM].
[35] D. Blas, J. Lesgourgues, and T. Tram, JCAP 2011, 034–034 (2011).
[36] A. c. v. Slosar, Phys. Rev. D 73, 123501 (2006).
[37] A. Font-Ribera, P. McDonald, N. Mostek, B. A. Reid, H.-J. Seo, and A. Slosar, JCAP 05, 023 (2014), arXiv:1308.4164 [astro-ph.CO].
[38] E. Di Valentino et al. (CORE), JCAP 04, 017 (2018), arXiv:1612.00021 [astro-ph.CO].
[39] T. Damour, G. W. Gibbons, and C. Gundlach, Phys. Rev. Lett. 64, 123 (1990).
[40] M. Chevallier and D. Polarski, International Journal of Modern Physics D 10, 213 (2001).
[41] E. Linder, Physical review letters 90, 091301 (2003).
[42] N. J. Nunes, AIP Conf. Proc. 736, 135 (2004).
[43] J. Lesgourgues, G. Mangano, G. Miele, and S. Pastor, Neutrino Cosmology (Cambridge University Press, 2013).
[44] T. Barreiro, E. J. Copeland, and N. J. Nunes, Phys. Rev. D 61, 127301 (2000).
[45] E. Lifshitz, J. Phys. (USSR) 10, 116 (1946).
[46] C.-P. Ma and E. Bertschinger, Astrophys. J. 455, 7 (1995), arXiv:astro-ph/9506072.
[47] J. Lesgourgues and T. Tram, Journal of Cosmology and Astroparticle Physics 2011, 032 (2011).
[48] L. Amendola, Mon. Not. Roy. Astron. Soc. 312, 521 (2000), arXiv:astro-ph/9906073.
[49] J. Lesgourgues, L. Perotto, S. Pastor, and M. Piat, Phys. Rev. D 73, 045021 (2006), arXiv:astroph/0511735.
[50] O. E. Bjaelde, A. W. Brookfield, C. van de Bruck, S. Hannestad, D. F. Mota, L. Schrempp, and D. Tocchini-Valentini, JCAP 01, 026 (2008), arXiv:0705.2018 [astro-ph].
[51] Planck Collaboration, Ade, P. A. R., Aghanim, N., et al., A&A 536, A1 (2011).
[52] D. J. ”Eisenstein and others” (SDSS), Astrophys. J. 633, 560 (2005), arXiv:astro-ph/0501171.
[53] S. Cole et al. (2dFGRS), Mon. Not. Roy. Astron. Soc. 362, 505 (2005), arXiv:astro-ph/0501174.
[54] W. J. Percival, S. Cole, D. J. Eisenstein, R. C. Nichol, J. A. Peacock, A. C. Pope, and A. S. Szalay, Mon. Not. Roy. Astron. Soc. 381, 1053 (2007), arXiv:0705.3323 [astro-ph].
[55] N. Aghanim et al. (Planck), Astron. Astrophys. 641, A8 (2020), arXiv:1807.06210 [astro-ph.CO].
[56] N. Aghanim et al. (Planck), Astron. Astrophys. 641, A5 (2020), arXiv:1907.12875 [astro-ph.CO].
[57] A. J. Ross, L. Samushia, C. Howlett, W. J. Percival, A. Burden, and M. Manera, Mon. Not. Roy. Astron. Soc. 449, 835 (2015), arXiv:1409.3242 [astro-ph.CO].
[58] C. P. Ahn et al., The Astrophysical Journal Supplement Series 203, 21 (2012).
[59] F. Beutler, C. Blake, M. Colless, D. H. Jones, L. Staveley-Smith, L. Campbell, Q. Parker, W. Saunders, and F. Watson, Monthly Notices of the Royal Astronomical Society 416, 3017 (2011).
[60] J. Froustey, C. Pitrou, and M. C. Volpe, JCAP 12, 015 (2020), arXiv:2008.01074 [hep-ph].
[61] J. J. Bennett, G. Buldgen, P. F. De Salas, M. Drewes, S. Gariazzo, S. Pastor, and Y. Y. Y. Wong, JCAP 04, 073 (2021), arXiv:2012.02726 [hep-ph].
[62] B. Audren, J. Lesgourgues, K. Benabed, and S. Prunet, JCAP 2013, 001 (2013), arXiv:1210.7183 [astro-ph.CO].
[63] T. Brinckmann and J. Lesgourgues, Physics of the Dark Universe 24, 100260 (2019).
[64] A. Lewis, “GetDist: Monte Carlo sample analyzer,” Astrophysics Source Code Library, record ascl:1910.018 (2019), arXiv:1910.13970 [astro-ph.IM].
[65] A. G´omez-Valent, Z. Zheng, L. Amendola, V. Pettorino, and C. Wetterich, Phys. Rev. D 104, 083536 (2021), arXiv:2107.11065 [astro-ph.CO].
[66] A. G´omez-Valent, Z. Zheng, L. Amendola, C. Wetterich, and V. Pettorino, Phys. Rev. D 106, 103522 (2022), arXiv:2207.14487 [astro-ph.CO].
[67] S. Alam et al. (eBOSS), Phys. Rev. D 103, 083533 (2021), arXiv:2007.08991 [astro-ph.CO].
[68] A. Amon et al. (DES), Phys. Rev. D 105, 023514 (2022), arXiv:2105.13543 [astro-ph.CO].
[69] T. M. C. Abbott et al. (Kilo-Degree Survey, DES), (2023), arXiv:2305.17173 [astro-ph.CO].
[70] L. F. Secco et al. (DES), Phys. Rev. D 105, 023515 (2022), arXiv:2105.13544 [astro-ph.CO].
[71] V. Poulin, T. L. Smith, T. Karwal, and M. Kamionkowski, Phys. Rev. Lett. 122, 221301 (2019), arXiv:1811.04083 [astro-ph.CO].
[72] D. H. F. de Souza and R. Rosenfeld, (2023), arXiv:2302.04644 [astro-ph.CO].
[73] P. Brax, C. van de Bruck, E. Di Valentino, W. Giar`e, and S. Trojanowski, (2023), arXiv:2303.16895 [astroph.CO].
[74] P. Brax, C. van de Bruck, E. Di Valentino, W. Giar`e, and S. Trojanowski, Phys. Dark Univ. 42, 101321 (2023), arXiv:2305.01383 [astro-ph.CO].
[75] F. J. Qu et al. (ACT), (2023), arXiv:2304.05202 [astro-ph.CO].
[76] H. Hildebrandt et al., Mon. Not. Roy. Astron. Soc. 465, 1454 (2017), arXiv:1606.05338 [astro-ph.CO].
L O A D I N G
. . . comments & more!
. . . comments & more!
