Astrophysical cosmology

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The last several years have seen a tremendous ferment of activity in astrophysical cosmology. Much of the theoretical impetus has come from particle physics theories of the early universe and candidates for dark matter, but what promise to be even more significant are improved direct observations of high z galaxies and intergalactic matter, deeper and more comprehensive redshift surveys, and the increasing power of computer simulations of the dynamical evolution of large scale structure. Upper limits on the anisotropy of the microwave background radiation are gradually getting tighter and constraining more severely theoretical scenarios for the evolution of the universe. … continued below

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10 pages

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Bardeen, J.M. January 1, 1986.

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Description

The last several years have seen a tremendous ferment of activity in astrophysical cosmology. Much of the theoretical impetus has come from particle physics theories of the early universe and candidates for dark matter, but what promise to be even more significant are improved direct observations of high z galaxies and intergalactic matter, deeper and more comprehensive redshift surveys, and the increasing power of computer simulations of the dynamical evolution of large scale structure. Upper limits on the anisotropy of the microwave background radiation are gradually getting tighter and constraining more severely theoretical scenarios for the evolution of the universe. 47 refs.

Physical Description

10 pages

Notes

NTIS, PC A02/MF A01; 1.

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  • 11. international conference on general relativity and gravitation, Stockholm, Sweden, 1 Jul 1986

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  • Other: DE87008239
  • Report No.: CONF-8607113-3
  • Grant Number: AC06-81ER40048
  • Office of Scientific & Technical Information Report Number: 6541430
  • Archival Resource Key: ark:/67531/metadc1200211

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Office of Scientific & Technical Information Technical Reports

Reports, articles and other documents harvested from the Office of Scientific and Technical Information.

Office of Scientific and Technical Information (OSTI) is the Department of Energy (DOE) office that collects, preserves, and disseminates DOE-sponsored research and development (R&D) results that are the outcomes of R&D projects or other funded activities at DOE labs and facilities nationwide and grantees at universities and other institutions.

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Creation Date

  • January 1, 1986

Added to The UNT Digital Library

  • July 3, 2018, 8:14 a.m.

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  • June 10, 2019, 11:33 a.m.

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Bardeen, J.M. Astrophysical cosmology, article, January 1, 1986; United States. (https://digital.library.unt.edu/ark:/67531/metadc1200211/: accessed March 28, 2024), University of North Texas Libraries, UNT Digital Library, https://digital.library.unt.edu; crediting UNT Libraries Government Documents Department.

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