Neutrino physics from the cosmic microwave background and large scale structure

被引：226

作者：

Abazajian, K. N. ^{[1
]}

Arnold, K. ^{[2
]}

Austermann, J. ^{[3
]}

Benson, B. A. ^{[4
]}

Bischoff, C. ^{[5
]}

Bock, J. ^{[6
]}

Bond, J. R. ^{[7
]}

Borrill, J. ^{[8
]}

Calabrese, E. ^{[9
]}

Carlstrom, J. E. ^{[4
]}

Carvalho, C. S. ^{[10
]}

Chang, C. L.

Chiang, H. C. ^{[11
]}

Church, S. ^{[12
]}

Cooray, A. ^{[1
]}

'Crawford, T. M. ^{[4
]}

Dawson, K. S. ^{[13
]}

Das, S. ^{[14
]}

Devlin, M. J. ^{[15
]}

Dobbs, M. ^{[16
]}

Dodelson, S. ^{[17
]}

Dore, O. ^{[18
]}

Dunkley, J. ^{[9
]}

Errard, J. ^{[19
]}

Fraisse, A. ^{[20
]}

Gallicchio, J. ^{[4
]}

Halverson, N. W. ^{[3
]}

Hanany, S. ^{[21
]}

Hildebrandt, S. R. ^{[6
]}

Hincks, A. ^{[22
]}

Hlozek, R. ^{[23
]}

Holder, G. ^{[16
]}

Holzapfel, W. L. ^{[24
]}

Honscheid, K. ^{[25
]}

Hu, W. ^{[4
]}

Hubmayr, J. ^{[26
]}

Irwin, K. ^{[27
]}

Jones, W. C. ^{[20
]}

Kamionkowski, M. ^{[28
]}

Keating, B. ^{[2
]}

Keisler, R. ^{[4
]}

Knox, L. ^{[29
]}

Komatsu, E. ^{[30
]}

Kovac, J. ^{[5
]}

Kuo, C. -L. ^{[27
]}

Lawrence, C. ^{[18
]}

Lee, A. T. ^{[24
]}

Leitch, E. ^{[31
]}

Linder, E. ^{[32
]}

Lubin, P. ^{[33
]}

机构：

[1] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

[2] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA

[3] Univ Colorado, Dept Astrophys & Planetary Sci, Boulder, CO 80309 USA

[4] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA

[5] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

[6] CALTECH, Dept Phys, Pasadena, CA 91125 USA

[7] Univ Toronto, Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada

[8] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94720 USA

[9] Univ Oxford, Subdept Astrophys, Oxford OX1 3RH, England

[10] Univ Lisbon, Ctr Astron & Astrofis, P-1349018 Lisbon, Portugal

[11] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, ZA-4000 Durban, South Africa

[12] Stanford Univ, Dept Phys, Stanford, CA 94305 USA

[13] Univ Utah, Dept Phys & Astron, Salt Lake City, UT 84112 USA

[14] Argonne Natl Lab, Dept High Energy Phys, Lemont, IL 60439 USA

[15] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA

[16] McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada

[17] Fermilab Natl Accelerator Lab, Fermilab Ctr Particle Astrophys, Batavia, IL 60510 USA

[18] CALTECH, Jet Prop Lab, Pasadena, CA USA

[19] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA

[20] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA

[21] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA

[22] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z4, Canada

[23] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA

[24] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[25] Ohio State Univ, Dept Phys, Columbus, OH 43210 USA

[26] NIST, Quantum Devices Grp, Boulder, CO 80305 USA

[27] Stanford Univ, Dept Phys, Stanford, CA 94305 USA

[28] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA

[29] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA

[30] Max Planck Inst Astrophys, D-85741 Garching, Germany

[31] Univ Chicago, Chicago, IL 60637 USA

[32] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA

[33] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA

[34] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA

[35] Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA

[36] Princeton Univ, Joseph Henry Labs Phys, Princeton, NJ 08544 USA

[37] Cornell Univ, Dept Phys, Ithaca, NY 14853 USA

[38] Case Western Reserve Univ, Dept Phys, Ctr Educ & Res Cosmol & Astrophys, Cleveland, OH 44106 USA

[39] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA

[40] Brookhaven Natl Lab, Upton, NY 11375 USA

[41] Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada

[42] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA

[43] Univ Paris Diderot, CEA Irfu, Observ Paris, Sorbonne Paris Cite,APC,CNRS IN2P3, F-75205 Paris, France

[44] Syracuse Univ, Dept Phys, Syracuse, NY 13244 USA

[45] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

来源：

ASTROPARTICLE PHYSICS | 2015年 / 63卷

基金：

美国国家科学基金会;

关键词：

Neutrinos; Cosmology; Cosmic microwave background; Large scale structure; OSCILLATION SPECTROSCOPIC SURVEY; POWER-SPECTRUM; WEIGHING NEUTRINOS; GALAXIES; TELESCOPE; SYSTEMATICS; COSMOLOGY; BARYONS; MATTER;

D O I：

10.1016/j.astropartphys.2014.05.014

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

This is a report on the status and prospects of the quantification of neutrino properties through the cosmological neutrino background for the Cosmic Frontier of the Division of Particles and Fields Community Summer Study long-term planning exercise. Experiments planned and underway are prepared to study the cosmological neutrino background in detail via its influence on distance-redshift relations and the growth of structure. The program for the next decade described in this document, including upcoming spectroscopic galaxy surveys eBOSS and DESI and a new Stage-IV CMB polarization experiment CMB-S4, will achieve sigma(sigma m(v)) = 16 meV and sigma(N-eff)= 0.020. Such a mass measurement will produce a high significance detection of non-zero sigma m(v), whose lower bound derived from atmospheric and solar neutrino oscillation data is about 58 meV. If neutrinos have a minimal normal mass hierarchy, this measurement will definitively rule out the inverted neutrino mass hierarchy, shedding light on one of the most puzzling aspects of the Standard Model of particle physics - the origin of mass. This precise a measurement of N-eff will allow for high sensitivity to any light and dark degrees of freedom produced in the big bang and a precision test of the standard cosmological model prediction that N-eff = 3.046. (C) 2014 Elsevier B.V. All rights reserved.

引用

页码：66 / 80

页数：15

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