Constraints on the sum of neutrino masses using cosmological data including the latest extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample

Sai Wang; Yi-Fan Wang; Dong-Mei Xia

doi:10.1088/1674-1137/42/6/065103

Chinese Physics C> 2018, Vol. 42> Issue(6) : 065103 DOI: 10.1088/1674-1137/42/6/065103

Constraints on the sum of neutrino masses using cosmological data including the latest extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample

1.
Department of Physics, The Chinese University of Hong Kong, Shatin, N. T., Hong Kong SAR 999077, China
2.
Key Laboratory of Low-grade Energy Utilization Technologies &

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Abstract：
We investigate the constraints on the sum of neutrino masses (Σm_ν) using the most recent cosmological data, which combines the distance measurement from baryonic acoustic oscillation in the extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample with the power spectra of temperature and polarization anisotropies in the cosmic microwave background from the Planck 2015 data release. We also use other low-redshift observations, including the baryonic acoustic oscillation at relatively low redshifts, Type Ia supernovae, and the local measurement of the Hubble constant. In the standard cosmological constant Λ cold dark matter plus massive neutrino model, we obtain the 95% upper limit to be Σm_ν<0.129 eV for the degenerate mass hierarchy, Σm_ν<0.159 eV for the normal mass hierarchy, and Σm_ν<0.189 eV for the inverted mass hierarchy. Based on Bayesian evidence, we find that the degenerate hierarchy is positively supported, and the current data combination cannot distinguish between normal and inverted hierarchies. Assuming the degenerate mass hierarchy, we extend our study to non-standard cosmological models including generic dark energy, spatial curvature, and extra relativistic degrees of freedom, but find these models are not favored by the data.
- neutrino mass ,
- mass hierarchy ,
- cosmological constraints

References

[1]	C. Patrignani et al (Particle Data Group), Chin. Phys. C, 40(10): 100001 (2016)
[2]	V. N. Aseev et al (Troitsk Collaboration), Phys. Rev. D, 84: 112003 (2011) arXiv: 1108.5034 [hep-ex]
[3]	J. Lesgourgues and S. Pastor, Phys. Rept., 429: 307 (2006) astro-ph/0603494
[4]	Z. Hou et al, Astrophys. J., 782: 74 (2014) arXiv: 1212.6267 [astro-ph.CO]
[5]	P. A. R. Ade et al (Planck Collaboration), Astron. Astrophys., 594: A13 (2016) arXiv: 1502.01589 [astro-ph.CO]
[6]	W. Hu, D. J. Eisenstein, and M. Tegmark, Phys. Rev. Lett., 80: 5255 (1998) astro-ph/9712057
[7]	W. Hu and S. Dodelson, Ann. Rev. Astron. Astrophys., 40: 171 (2002) astro-ph/0110414
[8]	E. Komatsu et al (WMAP Collaboration), Astrophys. J. Suppl., 180: 330 (2009) arXiv: 0803.0547 [astro-ph]
[9]	B. A. Reid, L. Verde, R. Jimenez, and O. Mena, JCAP, 1001: 003 (2010) arXiv: 0910.0008 [astro-ph.CO]
[10]	S. A. Thomas, F. B. Abdalla, and O. Lahav, Phys. Rev. Lett., 105: 031301 (2010) arXiv: 0911.5291 [astro-ph.CO]
[11]	R. Jimenez, T. Kitching, C. Pena-Garay, and L. Verde, JCAP, 1005: 035 (2010) arXiv: 1003.5918 [astro-ph.CO]
[12]	M. E. C. Swanson, W. J. Percival, and O. Lahav, Mon. Not. Roy. Astron. Soc., 409: 1100 (2010) arXiv: 1006.2825 [astro-ph.CO]
[13]	S. Riemer-Sorensen, D. Parkinson, and T. M. Davis, Phys. Rev. D, 89: 103505 (2014) arXiv: 1306.4153 [astro-ph.CO]
[14]	G. Rossi, C. Yche, N. Palanque-Delabrouille, and J. Lesgourgues, Phys. Rev. D, 92(6): 063505 (2015) arXiv: 1412.6763 [astro-ph.CO]
[15]	N. Palanque-Delabrouille et al, JCAP, 1511(11): 011 (2015) arXiv: 1506.05976 [astro-ph.CO]
[16]	E. Di Valentino, E. Giusarma, O. Mena, A. Melchiorri, and J. Silk, Phys. Rev. D, 93(8): 083527 (2016) arXiv: 1511.00975 [astro-ph.CO]
[17]	A. J. Cuesta, V. Niro, and L. Verde, Phys. Dark Univ., 13: 77 (2016) arXiv: 1511.05983 [astro-ph.CO]
[18]	L. Xu and Q. G. Huang, Sci. China Phys. Mech. Astron., 61(3): 039521 (2018) arXiv: 1611.05178 [astro-ph.CO]
[19]	F. Capozzi, E. Di Valentino, E. Lisi, A. Marrone, A. Melchiorri, and A. Palazzo, Phys. Rev. D, 95(9): 096014 (2017) arXiv: 1703.04471 [hep-ph]
[20]	S. Hannestad and T. Schwetz, JCAP, 1611(11): 035 (2016) arXiv: 1606.04691 [astro-ph.CO]
[21]	A. Caldwell, A. Merle, O. Schulz, and M. Totzauer, Phys. Rev. D, 96(7): 073001 (2017) arXiv: 1705.01945 [hep-ph]
[22]	Q. G. Huang, K. Wang, and S. Wang, Eur. Phys. J. C, 76(9): 489 (2016) arXiv: 1512.05899 [astro-ph.CO]
[23]	F. Beutler et al, Mon. Not. Roy. Astron. Soc., 416: 3017 (2011) arXiv: 1106.3366 [astro-ph.CO]
[24]	A. J. Ross, L. Samushia, C. Howlett, W. J. Percival, A. Burden, and M. Manera, Mon. Not. Roy. Astron. Soc., 449(1): 835 (2015) arXiv: 1409.3242 [astro-ph.CO]
[25]	H. Gil-Marin et al, Mon. Not. Roy. Astron. Soc., 460(4): 4210 (2016) arXiv: 1509.06373 [astro-ph.CO]
[26]	E. Giusarma, M. Gerbino, O. Mena, S. Vagnozzi, S. Ho, and K. Freese, Phys. Rev. D, 94(8): 083522 (2016) arXiv: 1605.04320 [astro-ph.CO]
[27]	S. Vagnozzi, E. Giusarma, O. Mena, K. Freese, M. Gerbino, S. Ho, and M. Lattanzi, Phys. Rev. D, 96(12): 123503 (2017) arXiv: 1701.08172 [astro-ph.CO]
[28]	S. Wang, Y. F. Wang, D. M. Xia, and X. Zhang, Phys. Rev. D, 94(8): 083519 (2016) arXiv: 1608.00672 [astro-ph.CO]
[29]	E. K. Li, H. Zhang, M. Du, Z. H. Zhou, and L. Xu, arXiv: 1703.01554 [astro-ph.CO]
[30]	E. Di Valentino, E. Giusarma, M. Lattanzi, O. Mena, A. Melchiorri, and J. Silk, Phys. Lett. B, 752: 182 (2016) arXiv: 1507.08665 [astro-ph.CO]
[31]	X. Zhang, Phys. Rev. D, 93(8): 083011 (2016) arXiv: 1511.02651 [astro-ph.CO]
[32]	R. Allison, P. Caucal, E. Calabrese, J. Dunkley, and T. Louis, Phys. Rev. D, 92(12): 123535 (2015) arXiv: 1509.07471 [astro-ph.CO]
[33]	M. Gerbino, M. Lattanzi, and A. Melchiorri, Phys. Rev. D, 93(3): 033001 (2016) arXiv: 1507.08614 [hep-ph]
[34]	M. M. Zhao, Y. H. Li, J. F. Zhang, and X. Zhang, Mon. Not. Roy. Astron. Soc., 469: 1713 (2017) arXiv: 1608.01219 [astro-ph.CO]
[35]	M. Gerbino, K. Freese, S. Vagnozzi, M. Lattanzi, O. Mena, E. Giusarma, and S. Ho, Phys. Rev. D, 95(4): 043512 (2017) arXiv: 1610.08830 [astro-ph.CO]
[36]	W. Yang, R. C. Nunes, S. Pan, and D. F. Mota, Phys. Rev. D, 95(10): 103522 (2017) arXiv: 1703.02556 [astro-ph.CO]
[37]	M. Ata et al, Mon. Not. Roy. Astron. Soc., 473(4): 4773 (2018) arXiv: 1705.06373 [astro-ph.CO]
[38]	G. B. Zhao et al, Mon. Not. Roy. Astron. Soc., 457(3): 2377 (2016) arXiv: 1510.08216 [astro-ph.CO]
[39]	A. Lewis and A. Challinor, Phys. Rept., 429: 1 (2006) astro-ph/0601594.
[40]	M. Betoule et al (SDSS Collaboration), Astron. Astrophys., 568: A22 (2014) arXiv: 1401.4064 [astro-ph.CO]
[41]	A. G. Riess et al, Astrophys. J., 826(1): 56 (2016) arXiv: 1604.01424 [astro-ph.CO]
[42]	C. Heymans et al, Mon. Not. Roy. Astron. Soc., 427: 146 (2012) arXiv: 1210.0032 [astro-ph.CO]
[43]	T. Erben et al, Mon. Not. Roy. Astron. Soc., 433: 2545 (2013) arXiv: 1210.8156 [astro-ph.CO]
[44]	L. Samushia et al, Mon. Not. Roy. Astron. Soc., 439(4): 3504 (2014) arXiv: 1312.4899 [astro-ph.CO]
[45]	P. A. R. Ade et al (Planck Collaboration), Astron. Astrophys., 571: A20 (2014) arXiv: 1303.5080 [astro-ph.CO]
[46]	A. Lewis and S. Bridle, Phys. Rev. D, 66: 103511 (2002) astro-ph/0205436.
[47]	W. J. Handley, M. P. Hobson, and A. N. Lasenby, Mon. Not. Roy. Astron. Soc., 450(1): L61 (2015) arXiv: 1502.01856 [astro-ph.CO]
[48]	W. J. Handley, M. P. Hobson, and A. N. Lasenby, Mon. Not. Roy. Astron. Soc., 453(4): 4384 (2015) arXiv: 1506.00171 [astro-ph.IM]
[49]	R. E. Kass, and A. E. Raftery. Journal of the American Statistical Association, 90(430): 773-795 (1995)
[50]	K. N. Abazajian et al (Topical Conveners: K.N. Abazajian, J.E. Carlstrom, A.T. Lee Collaboration), Astropart. Phys., 63: 66 (2015) arXiv: 1309.5383 [astro-ph.CO]
[51]	Y. Chen, B. Ratra, M. Biesiada, S. Li, and Z. H. Zhu, Astrophys. J., 829(2): 61 (2016) arXiv: 1603.07115 [astro-ph.CO]
[52]	A. Font-Ribera, P. McDonald, N. Mostek, B. A. Reid, H. J. Seo, and A. Slosar, JCAP, 1405: 023 (2014) arXiv: 1308.4164 [astro-ph.CO]
[53]	E. Calabrese et al, JCAP, 1408: 010 (2014) arXiv: 1406.4794 [astro-ph.CO]
[54]	B. A. Benson et al (SPT-3G Collaboration), Proc. SPIE Int. Soc. Opt. Eng., 9153: 91531P (2014) arXiv: 1407.2973 [astro-ph.IM]
[55]	T. Matsumura et al, J. Low. Temp. Phys., 176: 733 (2014) arXiv: 1311.2847 [astro-ph.IM]
[56]	A. Kogut et al, JCAP, 1107: 025 (2011) arXiv: 1105.2044 [astro-ph.CO]
[57]	P. A. Abell et al (LSST Science and LSST Project Collaborations], arXiv: 0912.0201 [astro-ph.IM]
[58]	R. Laureijs et al (EUCLID Collaboration), arXiv: 1110.3193 [astro-ph.CO]
[59]	A. Liu, J. R. Pritchard, R. Allison, A. R. Parsons, U. Seljak, and B. D. Sherwin, Phys. Rev. D, 93(4): 043013 (2016) arXiv: 1509.08463 [astro-ph.CO]

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Sai Wang, Yi-Fan Wang and Dong-Mei Xia. Constraints on the sum of neutrino masses using cosmological data including the latest extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample[J]. Chinese Physics C, 2018, 42(6): 065103. doi: 10.1088/1674-1137/42/6/065103

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Received: 2018-02-22

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SW is Supported by a grant from the Research Grant Council of the Hong Kong Special Administrative Region, China (14301214), DMX is Supported by the National Natural Science Foundation of China (11505018) and the Chongqing Science and Technology Plan Project (Cstc2015jvyj40031)

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Constraints on the sum of neutrino masses using cosmological data including the latest extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample

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Constraints on the sum of neutrino masses using cosmological data including the latest extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample

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