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Title: Neutrino Physics from the Cosmic Microwave Background and Large Scale Structure

Abstract

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 σ(σmν) = 16 meV and σ(Neff) = 0.020. Such a mass measurement will produce a high significance detection of non-zero σmν, 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 Neff 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 predictionmore » that Neff = 3.046.« less

Authors:
 [1];  [2];  [3];  [4];  [5];  [6];  [7];  [8];  [9];  [4];  [10];  [4];  [11];  [12];  [1];  [4];  [13];  [14];  [15];  [16] more »;  [17];  [18];  [9];  [19];  [20];  [4];  [3];  [21];  [6];  [22];  [23];  [16];  [24];  [25];  [4];  [26];  [12];  [20];  [27];  [2];  [4];  [28];  [29];  [5];  [12];  [18];  [24];  [30];  [31];  [32];  [33];  [34];  [35];  [36];  [17];  [18];  [35];  [21];  [25];  [37];  [38];  [25];  [7];  [12];  [39];  [40];  [41];  [35];  [5];  [42];  [4];  [14];  [43];  [44]; ;  [12];  [24] « less
  1. Univ. of California, Irvine, CA (United States). Dept. of Physics and Astronomy
  2. Univ. of California, San Diego, CA (United States). Dept. of Physics
  3. Univ. of Colorado, Boulder, CO (United States). Dept. of Astrophysical and Planetary Sciences
  4. Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP)
  5. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
  6. California Inst. of Technology (CalTech), Pasadena, CA (United States). Dept. of Physics
  7. Univ. of Toronto, ON (Canada). Canadian Inst. for Theoretical Astrophysics
  8. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). Computational Cosmology Center
  9. Univ. of Oxford (United Kingdom). Sub-dept. of Astrophysics
  10. Univ. of Lisbon (Portugal). Centro de Astronomia e Astrofisica
  11. Univ. of KwaZulu-Natal, Durban (South Africa). Astrophysics & Cosmology Research Unit. School of Mathematics, Statistics & Computer Science
  12. Stanford Univ., CA (United States). Dept. of Physics
  13. Univ. of Utah, Salt Lake City, UT (United States). Dept. of Physics and Astronomy
  14. Argonne National Lab. (ANL), Argonne, IL (United States). Dept. of High Energy Physics
  15. Univ. of Pennsylvania, Philadelphia, PA (United States). Dept. of Physics and Astronomy
  16. McGill Univ., Montreal, QC (Canada). Dept of Physics
  17. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States). Fermilab Center for Particle Astrophysics
  18. California Inst. of Technology (CalTech), Pasadena, CA (United States). Jet Propulsion Lab.
  19. Univ. of California, Berkeley, CA (United States). Space Sciences Lab.
  20. Princeton Univ., NJ (United States). Dept. of Physics
  21. Univ. of Minnesota, Minneapolis, MN (United States). School of Physics and Astronomy
  22. Univ. of British Columbia, Vancouver, BC (Canada). Dept. of Physics and Astronomy
  23. Princeton Univ., NJ (United States). Dept. of Astrophysical Sciences
  24. Univ. of California, Berkeley, CA (United States). Dept. of Physics
  25. The Ohio State Univ., Columbus, OH (United States). Dept of Physics
  26. National Inst. of Standards and Technology (NIST), Boulder, CO (United States). Quantum Devices Group
  27. Johns Hopkins Univ., Baltimore, MD (United States). Department of Physics and Astronomy
  28. Univ. of California, Davis, CA (United States). Dept. of Physics
  29. Max Planck Society, Garching (Germany). Max Planck Inst. for Astrophysik
  30. Univ. of Chicago, IL (United States)
  31. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
  32. Univ. of California, Santa Barbara, CA (United States). Dept. of Physics
  33. Univ. of Michigan, Ann Arbor, MI (United States). Dept. of Physics
  34. Columbia Univ., New York, NY (United States). Columbia Astrophysics Lab.
  35. Princeton Univ., NJ (United States). Joseph Henry Lab. of Physics
  36. Cornell Univ., Ithaca, NY (United States). Dept. of Physics
  37. Case Western Reserve Univ., Cleveland, OH (United States). Center for Education and Research in Cosmology and Astrophysics and Physics Dept.
  38. Stony Brook Univ., NY (United States). Dept. of Physics and Astronomy
  39. Brookhaven National Lab. (BNL), Upton, NY (United States)
  40. Perimeter Inst. for Theoretical Physics, Waterloo, ON (Canada)
  41. Princeton Univ., NJ (United States). Dept. of Astrophysical Science
  42. CNRS/IN2P3. Univ. Paris (France). Observatoire de Paris. AstroParticule et Cosmologie (APC)
  43. Syracuse Univ., NY (United States). Dept. of Physics
  44. NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
Publication Date:
Research Org.:
Brookhaven National Lab. (BNL), Upton, NY (United States); Argonne National Lab. (ANL), Argonne, IL (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP)
Contributing Org.:
Topical Conveners: K.N. Abazajian, J.E. Carlstrom, A.T. Lee
OSTI Identifier:
1172077
Alternate Identifier(s):
OSTI ID: 1335009; OSTI ID: 1524021
Report Number(s):
BNL-107333-2015-JA; FERMILAB-PUB-13-438-A; arXiv:1309.5383
Journal ID: ISSN 0927-6505; KA2301020; TRN: US1500480
Grant/Contract Number:  
SC00112704; AC02-07CH11359; AC02-05CH11231
Resource Type:
Accepted Manuscript
Journal Name:
Astroparticle Physics
Additional Journal Information:
Journal Volume: 63; Journal ID: ISSN 0927-6505
Publisher:
Elsevier
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Neutrinos; Cosmology; Cosmic microwave background; Large scale structure; 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS

Citation Formats

Abazajian, K. N., Arnold, K., Austermann, J., Benson, B. A., Bischoff, C., Bock, J., Bond, J. R., Borrill, J., Calabrese, E., Carlstrom, J. E., Carvalho, C. S., Chang, C. L., Chiang, H. C., Church, S., Cooray, A., Crawford, T. M., Dawson, K. S., Das, S., Devlin, M. J., Dobbs, M., Dodelson, S., Dore, O., Dunkley, J., Errard, J., Fraisse, A., Gallicchio, J., Halverson, N. W., Hanany, S., Hildebrandt, S. R., Hincks, A., Hlozek, R., Holder, G., Holzapfel, W. L., Honscheid, K., Hu, W., Hubmayr, J., Irwin, K., Jones, W. C., Kamionkowski, M., Keating, B., Keisler, R., Knox, L., Komatsu, E., Kovac, J., Kuo, C. -L., Lawrence, C., Lee, A. T., Leitch, E., Linder, E., Lubin, P., McMahon, J., Miller, A., Newburgh, L., Niemack, M. D., Nguyen, H., Nguyen, H. T., Page, L., Pryke, C., Reichardt, C. L., Ruhl, J. E., Sehgal, N., Seljak, U., Sievers, J., Silverstein, E., Slosar, A., Smith, K. M., Spergel, D., Staggs, S. T., Stark, A., Stompor, R., Vieregg, A. G., Wang, G., Watson, S., Wollack, E. J., W. Wu, Yoon, K. W., and Zahn, O. Neutrino Physics from the Cosmic Microwave Background and Large Scale Structure. United States: N. p., 2014. Web. doi:10.1016/j.astropartphys.2014.05.014.
Abazajian, K. N., Arnold, K., Austermann, J., Benson, B. A., Bischoff, C., Bock, J., Bond, J. R., Borrill, J., Calabrese, E., Carlstrom, J. E., Carvalho, C. S., Chang, C. L., Chiang, H. C., Church, S., Cooray, A., Crawford, T. M., Dawson, K. S., Das, S., Devlin, M. J., Dobbs, M., Dodelson, S., Dore, O., Dunkley, J., Errard, J., Fraisse, A., Gallicchio, J., Halverson, N. W., Hanany, S., Hildebrandt, S. R., Hincks, A., Hlozek, R., Holder, G., Holzapfel, W. L., Honscheid, K., Hu, W., Hubmayr, J., Irwin, K., Jones, W. C., Kamionkowski, M., Keating, B., Keisler, R., Knox, L., Komatsu, E., Kovac, J., Kuo, C. -L., Lawrence, C., Lee, A. T., Leitch, E., Linder, E., Lubin, P., McMahon, J., Miller, A., Newburgh, L., Niemack, M. D., Nguyen, H., Nguyen, H. T., Page, L., Pryke, C., Reichardt, C. L., Ruhl, J. E., Sehgal, N., Seljak, U., Sievers, J., Silverstein, E., Slosar, A., Smith, K. M., Spergel, D., Staggs, S. T., Stark, A., Stompor, R., Vieregg, A. G., Wang, G., Watson, S., Wollack, E. J., W. Wu, Yoon, K. W., & Zahn, O. Neutrino Physics from the Cosmic Microwave Background and Large Scale Structure. United States. https://doi.org/10.1016/j.astropartphys.2014.05.014
Abazajian, K. N., Arnold, K., Austermann, J., Benson, B. A., Bischoff, C., Bock, J., Bond, J. R., Borrill, J., Calabrese, E., Carlstrom, J. E., Carvalho, C. S., Chang, C. L., Chiang, H. C., Church, S., Cooray, A., Crawford, T. M., Dawson, K. S., Das, S., Devlin, M. J., Dobbs, M., Dodelson, S., Dore, O., Dunkley, J., Errard, J., Fraisse, A., Gallicchio, J., Halverson, N. W., Hanany, S., Hildebrandt, S. R., Hincks, A., Hlozek, R., Holder, G., Holzapfel, W. L., Honscheid, K., Hu, W., Hubmayr, J., Irwin, K., Jones, W. C., Kamionkowski, M., Keating, B., Keisler, R., Knox, L., Komatsu, E., Kovac, J., Kuo, C. -L., Lawrence, C., Lee, A. T., Leitch, E., Linder, E., Lubin, P., McMahon, J., Miller, A., Newburgh, L., Niemack, M. D., Nguyen, H., Nguyen, H. T., Page, L., Pryke, C., Reichardt, C. L., Ruhl, J. E., Sehgal, N., Seljak, U., Sievers, J., Silverstein, E., Slosar, A., Smith, K. M., Spergel, D., Staggs, S. T., Stark, A., Stompor, R., Vieregg, A. G., Wang, G., Watson, S., Wollack, E. J., W. Wu, Yoon, K. W., and Zahn, O. Sat . "Neutrino Physics from the Cosmic Microwave Background and Large Scale Structure". United States. https://doi.org/10.1016/j.astropartphys.2014.05.014. https://www.osti.gov/servlets/purl/1172077.
@article{osti_1172077,
title = {Neutrino Physics from the Cosmic Microwave Background and Large Scale Structure},
author = {Abazajian, K. N. and Arnold, K. and Austermann, J. and Benson, B. A. and Bischoff, C. and Bock, J. and Bond, J. R. and Borrill, J. and Calabrese, E. and Carlstrom, J. E. and Carvalho, C. S. and Chang, C. L. and Chiang, H. C. and Church, S. and Cooray, A. and Crawford, T. M. and Dawson, K. S. and Das, S. and Devlin, M. J. and Dobbs, M. and Dodelson, S. and Dore, O. and Dunkley, J. and Errard, J. and Fraisse, A. and Gallicchio, J. and Halverson, N. W. and Hanany, S. and Hildebrandt, S. R. and Hincks, A. and Hlozek, R. and Holder, G. and Holzapfel, W. L. and Honscheid, K. and Hu, W. and Hubmayr, J. and Irwin, K. and Jones, W. C. and Kamionkowski, M. and Keating, B. and Keisler, R. and Knox, L. and Komatsu, E. and Kovac, J. and Kuo, C. -L. and Lawrence, C. and Lee, A. T. and Leitch, E. and Linder, E. and Lubin, P. and McMahon, J. and Miller, A. and Newburgh, L. and Niemack, M. D. and Nguyen, H. and Nguyen, H. T. and Page, L. and Pryke, C. and Reichardt, C. L. and Ruhl, J. E. and Sehgal, N. and Seljak, U. and Sievers, J. and Silverstein, E. and Slosar, A. and Smith, K. M. and Spergel, D. and Staggs, S. T. and Stark, A. and Stompor, R. and Vieregg, A. G. and Wang, G. and Watson, S. and Wollack, E. J. and W. Wu and Yoon, K. W. and Zahn, O.},
abstractNote = {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 σ(σmν) = 16 meV and σ(Neff) = 0.020. Such a mass measurement will produce a high significance detection of non-zero σmν, 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 Neff 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 Neff = 3.046.},
doi = {10.1016/j.astropartphys.2014.05.014},
journal = {Astroparticle Physics},
number = ,
volume = 63,
place = {United States},
year = {2014},
month = {3}
}

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