Measuring dark matter power spectrum from cosmic microwave background

Physical Review Letters

Volumn 82, Issue 13, 1999, Pages 2636-2639

  Seljak, Uroš ^a,b   Zaldarriaga, Matias ^c  

^a PRINCETON UNIVERSITY   (United States)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^c INSTITUTE FOR ADVANCED STUDY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0041696834     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.82.2636     Document Type: Article

References (12)

1. M. A. Strauss, and J. A. Willick, Phys. Rep. 261, 271, (1995).
2. R. A. C. Croft, D. H. Weinberg, M. Pettini, L. Hernquist, and N. Katz, astro-ph/9809401.
3. R. D. Blandford, A. B. Saust, T. G. Brainerd, and J. V. Villumsen, Mon. Not. R. Astron. Soc. 251, 600, (1991).
4. J. Miralda-Escude, Astrophys. J. 380, 1, (1991).
5. N. Kaiser, Astrophys. J. 388, 272, (1992).
6. B. Jain, and U. Seljak, Astrophys. J. 484, 560, (1997).
7. L. Van Waerbeke, F. Bernardeau, and Y. Mellier, astro-ph/9807007.
8. F. Bernardeau, Astron. Astrophys. 324, 15, (1997). astro-ph/9802243.
9. M. Zaldarriaga, and U. Seljak, astro-ph/9810257.
10. U. Seljak, and M. Zaldarriaga, astro-ph/9811123.
11. D. Goldberg, and D. Spergel, astro-ph/9811251.
12. R. G. Crittenden, and N. G. Turok, Phys. Rev. Lett. 76, 575, (1996).