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Title: Growth of Cosmic Structure: Probing Dark Energy Beyond Expansion

The quantity and quality of cosmic structure observations have greatly accelerated in recent years, and further leaps forward will be facilitated by imminent projects. These will enable us to map the evolution of dark and baryonic matter density fluctuations over cosmic history. The way that these fluctuations vary over space and time is sensitive to several pieces of fundamental physics: the primordial perturbations generated by GUT-scale physics; neutrino masses and interactions; the nature of dark matter and dark energy. We focus on the last of these here: the ways that combining probes of growth with those of the cosmic expansion such as distance-redshift relations will pin down the mechanism driving the acceleration of the Universe.
 [1] ;  [2] ;  [3] ;  [4] ;  [5] ;  [6] ;  [1] ;  [7] ;  [7] ;  [8] ;  [9] ;  [10] ;  [11] ;  [8] ;  [12] ;  [13] ;  [14] ;  [10] ;  [14] ;  [15] more »;  [16] « less
  1. University of Michigan, Department of Physics Ann Harbor, MI (United States)
  2. UC Irvine, Department of Physics and Astronomy, CA (United States)
  3. Cornell University, Department of Astronomy, Ithaca, NY (United States)
  4. University of Washington, Department of Astronomy, Seattle, WA (United States)
  5. University of Utah, Department of Physics & Astronomy, Salt Lake City, UT (United States)
  6. Fermi National Accelerator Laboratory, Fermilab Center for Particle Astrophysics, Batavia, IL (United States); University of Chicago, Department of Physics & Astrophysics, Chicago, IL (United States)
  7. University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA (United States)
  8. Lawrence Berkeley National Laboratory, Physics Division, Berkeley, CA (United States)
  9. Carnegie Mellon University, Department of Physics, Pittsburgh, PA (United States)
  10. Brookhaven National Laboratory (BNL), Upton, NY (United States)
  11. California Institute of Technology, NASA Jet Propulsion Laboratory, Pasadena, CA (United States)
  12. SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
  13. Princeton University, Department of Astrophysical Sciences, Princeton, NJ (United States); Max-Planck-Insitute for Astrophysics, Garching (Germany)
  14. Stony Brook University, NY (United States)
  15. University of Michigan, Department of Physics, Ann Harbor, MI (United States)
  16. Chinese Academy of Science, National Astronomy Observatories, Beijing (China)
Publication Date:
Report Number(s):
BNL-107345-2015-JA; FERMILAB-PUB-13-439-A; arXiv:1309.5385
Journal ID: ISSN 0927-6505; KA2301020; TRN: US1500482
Grant/Contract Number:
SC00112704; AC02-07CH11359
Accepted Manuscript
Journal Name:
Astroparticle Physics
Additional Journal Information:
Journal Volume: 63; Journal ID: ISSN 0927-6505
Research Org:
Brookhaven National Laboratory (BNL), Upton, NY (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Org:
USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
Country of Publication:
United States
79 ASTRONOMY AND ASTROPHYSICS; Cosmology; Large-scale structure; Dark energy
OSTI Identifier:
Alternate Identifier(s):
OSTI ID: 1335008