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Dark Matter Science in the Era of LSST

Journal Article · · No journal information
OSTI ID:1545118
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  1. Wisconsin U., Madison
  2. Chicago U., KICP; Fermilab; Chicago U.
  3. UC, Irvine
  4. Cambridge U., DAMTP
  5. KIPAC, Menlo Park
  6. New York U.
  7. Fermilab
  8. Durham U.
  9. LLNL, Livermore
  10. KASI, DaeJeon
  11. INFN, Trieste; SISSA, Trieste
  12. KIPAC, Menlo Park; SLAC
  13. U. Amsterdam, GRAPPA; Leiden U.
  14. Johns Hopkins U.
  15. Portsmouth U., ICG
  16. UC, Riverside
  17. UCLA
  18. Stockholm U., OKC
  19. Trieste Observ.
  20. EPFL, Lausanne, LPPC
  21. Harvard-Smithsonian Ctr. Astrophys.
  22. LBL, Berkeley
  23. Toronto U., Astron. Dept.
  24. Arizona U., Astron. Dept. - Steward Observ.
  25. Rutgers U., Piscataway
  26. Stanford U., Phys. Dept.
  27. Perimeter Inst. Theor. Phys.
  28. Annecy, LAPTH
  29. NASA, Goddard
  30. UC, Berkeley
  31. Chicago U.; Chicago U., KICP
  32. Ohio U.
  33. U. Montpellier 2, LUPM
  34. Garching, Max Planck Inst., MPE
  35. Carnegie Mellon U.
  36. Annecy, LAPTH; RWTH Aachen U.
  37. Harvard U.; New Mexico U.
  38. Stanford U.
  39. Queensland U.
  40. Mexico U.
  41. Jodrell Bank
  42. Harvard U. (main)
  43. Caltech, JPL
  44. Harvard U.
  45. Nova Gorica U.
  46. U. Surrey (main)
  47. UC, Davis
  48. U. Oxford (main)
  49. Canadian Inst. Theor. Astrophys.
  50. Chicago U., KICP
  51. Chicago U., KICP; Fermilab
  52. Madrid, IFT
  53. Argonne
  54. Barry U.
  55. KIPAC, Menlo Park; SLAC; Stanford U.
  56. Florida U.; Princeton U.
  57. Rochester U.
  58. Guanajuato U.
  59. Haverford Coll.
  60. KIPAC, Menlo Park; Stanford U.
  61. CCA, New York
  62. Ohio State U.
  63. Toronto U., Astron. Dept.; U. Toronto, Dunlap Inst. Astron. Astrophys.
  64. Virginia Tech.
  65. Pennsylvania U.
  66. UC, Davis; Yonsei U.
  67. UC, Santa Cruz, Inst. Part. Phys.
  68. TIFR, Mumbai, Dept. Theor. Phys.
  69. Cambridge U., Inst. of Astron.; Carnegie Mellon U.
  70. Brown U.
  71. University Coll. London
  72. Tucson Optical Research
  73. U. Padua, Dept. Phys. Astron.
  74. UC, San Diego
  75. Princeton U.
  76. Stony Brook U.
  77. UC, Berkeley, Astron. Dept.
  78. Pittsburgh U.
  79. LBL, Berkeley; UC, Berkeley
  80. Kapteyn Astron. Inst., Groningen; Cambridge U., KICC; Groningen U.
  81. ICTP, Trieste
  82. New York U., CCPP
  83. Orsay, LAL
  84. Tokyo U., IPMU
  85. Siena Coll., Loudonville
  86. Wyoming U.
  87. Stanford U.; KIPAC, Menlo Park
  88. Caltech
  89. Yale U.
  90. Chicago U.; Chicago U., KICP; Fermilab
  91. Brookhaven
  92. Texas A-M
  93. Zurich, ETH; Canadian Inst. Theor. Astrophys.
  94. University Coll. London; Stockholm U., OKC
  95. Ohio State U.; Ohio State U., CCAPP; Ohio State U., Dept. Astron.
  96. INFN, Rome; Rome U.
  97. New Hampshire U.
  98. Surrey U.
  99. UC, Santa Cruz
  100. Baltimore, Space Telescope Sci.
  101. ICTP, Trieste; LIneA, Rio de Janeiro
  102. Sejong U.
  103. Kansas State U.
  104. Madrid, Autonoma U.
  105. Shanghai, Astron. Observ.
  106. Chicago U.
  107. Carnegie Inst. Observ.
  108. Michigan U.
  109. MIT
  110. INAF, Rome
  111. Duke U.
  112. Oxford U.
  113. Houston U.
  114. Syracuse U.
  115. Garching, Max Planck Inst.
  116. Edinburgh U.
+ Show Author Affiliations
Astrophysical observations currently provide the only robust, empirical measurements of dark matter. In the coming decade, astrophysical observations will guide other experimental efforts, while simultaneously probing unique regions of dark matter parameter space. This white paper summarizes astrophysical observations that can constrain the fundamental physics of dark matter in the era of LSST. We describe how astrophysical observations will inform our understanding of the fundamental properties of dark matter, such as particle mass, self-interaction strength, non-gravitational interactions with the Standard Model, and compact object abundances. Additionally, we highlight theoretical work and experimental/observational facilities that will complement LSST to strengthen our understanding of the fundamental characteristics of dark matter.
Research Organization:
Chicago U.; Oxford U.; Leiden U.; Stockholm U., OKC; U. Toronto, Dunlap Inst. Astron. Astrophys.; Guanajuato U.; NASA, Goddard; Arizona U., Astron. Dept. - Steward Observ.; Orsay, LAL; Wisconsin U., Madison; UC, Davis; Tucson Optical Research; LIneA, Rio de Janeiro; Yale U.; U. Amsterdam, GRAPPA; Perimeter Inst. Theor. Phys.; UC, Berkeley, Astron. Dept.; Rochester U.; Johns Hopkins U.; Trieste Observ.; Pennsylvania U.; Queensland U.; UC, San Diego; MIT; SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Stony Brook U.; INFN, Trieste; Cambridge U., DAMTP; Carnegie Inst. Observ.; EPFL, Lausanne, LPPC; UC, Santa Cruz, Inst. Part. Phys.; Wyoming U.; New Hampshire U.; Stanford U.; Annecy, LAPTH; Nova Gorica U.; Brookhaven National Laboratory (BNL), Upton, NY (United States); Harvard U. (main); Canadian Inst. Theor. Astrophys.; Groningen U.; Sejong U.; UC, Irvine; Garching, Max Planck Inst., MPE; CCA, New York; Ohio State U.; Siena Coll., Loudonville; UC, Berkeley; Yonsei U.; Syracuse U.; U. Surrey (main); Chicago U., KICP; TIFR, Mumbai, Dept. Theor. Phys.; U. Padua, Dept. Phys. Astron.; Edinburgh U.; New York U., CCPP; Michigan U.; Zurich, ETH; Jodrell Bank; Cambridge U., KICC; Florida U.; U. Oxford (main); Kapteyn Astron. Inst., Groningen; Princeton U.; KASI, DaeJeon; SISSA, Trieste; Harvard U.; UC, Riverside; Houston U.; Caltech, JPL; Garching, Max Planck Inst.; New York U.; UC, Santa Cruz; Brown U.; Texas A-M; INAF, Rome; Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States); Rutgers U., Piscataway; Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); Toronto U., Astron. Dept.; University Coll. London; Rome U.; Madrid, IFT; Ohio U.; Caltech; Ohio State U., Dept. Astron.; Harvard-Smithsonian Ctr. Astrophys.; Argonne National Laboratory (ANL), Argonne, IL (United States); INFN, Rome; Haverford Coll.; ICTP, Trieste; Mexico U.; Baltimore, Space Telescope Sci.; Duke U.; Kansas State U.; Madrid, Autonoma U.; Shanghai, Astron. Observ.; Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Pittsburgh U.; RWTH Aachen U.; Cambridge U., Inst. of Astron.; Carnegie Mellon U.; Tokyo U., IPMU; Virginia Tech.; U. Montpellier 2, LUPM; UCLA; Portsmouth U., ICG; Surrey U.; Durham U.; Barry U.; New Mexico U.; Stanford U., Phys. Dept.; Ohio State U., CCAPP
Sponsoring Organization:
US Department of Energy
DOE Contract Number:
AC02-07CH11359
OSTI ID:
1545118
Report Number(s):
FERMILAB-PUB-19-141-A-AE-CD; oai:inspirehep.net:1724441; arXiv:1903.04425
Journal Information:
No journal information, Journal Name: No journal information
Country of Publication:
United States
Language:
English

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72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
79 ASTRONOMY AND ASTROPHYSICS