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 &

Abstract
HTML
Reference
Related

PDF

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]

[1]	Ye-Huang Pang , Xue Zhang , Qing-Guo Huang . Cosmological constraints on neutrino mass within consistent cosmological models. Chinese Physics C, 2024, 48(6): 065102. doi: 10.1088/1674-1137/ad34c0
[2]	Junji Jia , Yaoguang Wang , Shun Zhou . On the possibility to determine neutrino mass hierarchy via supernova neutrinos with short-time characteristics. Chinese Physics C, 2019, 43(9): 095102. doi: 10.1088/1674-1137/43/9/095102
[3]	Wen Yin . Dark matter, neutrino mass, cutoff for cosmic-ray neutrino, and the Higgs boson invisible decay from a neutrino portal interaction. Chinese Physics C, 2019, 43(4): 045101. doi: 10.1088/1674-1137/43/4/045101
[4]	Guo-yuan Huang , Zhi-zhong Xing , Jing-yu Zhu . Correlation of normal neutrino mass ordering with upper octant of θ₂₃ and third quadrant of δ via RGE-induced μ-τ symmetry breaking. Chinese Physics C, 2018, 42(12): 123108. doi: 10.1088/1674-1137/42/12/123108
[5]	Ran Ding , Zhi-Long Han , Li Huang , Yi Liao . Phenomenology of colored radiative neutrino mass model and its implications on cosmic-ray observations. Chinese Physics C, 2018, 42(10): 103101. doi: 10.1088/1674-1137/42/10/103101
[6]	Rui-Yun Guo , Jing-Fei Zhang , Xin Zhang . Exploring neutrino mass and mass hierarchy in the scenario of vacuum energy interacting with cold dark matter. Chinese Physics C, 2018, 42(9): 095103. doi: 10.1088/1674-1137/42/9/095103
[7]	Yong-Chang Huang , Syeda Tehreem Iqbal , Zhen Lei , Wen-Yu Wang . Some new symmetric relations and prediction of left- and right-handed neutrino masses using Koide's relation. Chinese Physics C, 2017, 41(4): 043104. doi: 10.1088/1674-1137/41/4/043104
[8]	Zhi-zhong Xing , Jing-yu Zhu . Neutrino mass ordering and μ-τ reflection symmetry breaking. Chinese Physics C, 2017, 41(12): 123103. doi: 10.1088/1674-1137/41/12/123103
[9]	Jing Tang , Zhong-Ming Niu , Jian-You Guo . Influence of binding energies of electrons on nuclear mass predictions. Chinese Physics C, 2016, 40(7): 074102. doi: 10.1088/1674-1137/40/7/074102
[10]	Yujiang Bi , Hao Cai , Ying Chen , Ming Gong , Zhaofeng Liu , Hao-Xue Qiao , Yi-Bo Yang . Diquark mass differences from unquenched lattice QCD. Chinese Physics C, 2016, 40(7): 073106. doi: 10.1088/1674-1137/40/7/073106
[11]	Fa-Peng Huang , Yifu Cai , Hong Li , Xinmin Zhang . A possible interpretation of the Higgs mass by the cosmological attractive relaxion. Chinese Physics C, 2016, 40(11): 113103. doi: 10.1088/1674-1137/40/11/113103
[12]	Shun Zhou . Update on two-zero textures of the Majorana neutrino mass matrix in light of recent T2K, Super-Kamiokande and NOvA results. Chinese Physics C, 2016, 40(3): 033102. doi: 10.1088/1674-1137/40/3/033102
[13]	J. -B. Bueb . Mass excess of ⁶⁹Br and the rp process. Chinese Physics C, 2015, 39(9): 094103. doi: 10.1088/1674-1137/39/9/094103
[14]	XING Zhi-Zhong , ZHOU Ye-Ling . Geometry of the effective Majorana neutrino mass in the 0νββ decay. Chinese Physics C, 2015, 39(1): 011001. doi: 10.1088/1674-1137/39/1/011001
[15]	ZHAO Xian-Feng , JIA Huan-Yu . Transition density of the large mass hyperon star. Chinese Physics C, 2014, 38(1): 015101. doi: 10.1088/1674-1137/38/1/015101
[16]	PENG Jin-Song , ZHOU Li-Juan , MENG Cheng-Ju , PAN Ji-Huan , MA Wei-Xing , YUAN Tong-Quan . Ratio of a strange quark mass m_s to up or down quark mass m_u,d predicted by a quark propagator in the frameworkof the chiral perturbation theory. Chinese Physics C, 2013, 37(4): 043101. doi: 10.1088/1674-1137/37/4/043101
[17]	SHAN Hong-Yun , ZHANG Ai-Lin . D and D_s in mass loaded flux tube. Chinese Physics C, 2010, 34(1): 16-21. doi: 10.1088/1674-1137/34/1/003
[18]	HUANG Wen-Xue , XIAO Guo-Qing , WANG Yue , TIAN Yu-Lin , ZHU Zhi-Chao , XU Hu-Shan , ZHAN Wen-Long . High precision mass measurement and LPT. Chinese Physics C, 2008, 32(S2): 197-200.
[19]	Li Jin , Li Yushan , Qi Nading , Xue Shengtian , Wang Ping , Hu Tao , Ma Donghong , Zhang Jiawen , Zhu Qiming , Jiang Chunhua , Jiang Zhijin . Monte Carlo Study on the Strategy of Tau Mass Measurement. Chinese Physics C, 1995, 19(S2): 115-123.
[20]	HUANG Wu-Liang . Neutrino Mass and the Superstructure of the Universe. Chinese Physics C, 1991, 15(12): 1135-1136.

Access

Get Citation

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

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2018-02-22

Fund

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)

Article Metric

Article Views(1600)
PDF Downloads(12)
Cited by(0)

Policy on re-use

To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.

通讯作者: 陈斌, bchen63@163.com

1.
沈阳化工大学材料科学与工程学院沈阳 110142

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

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

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

HTML

目录