CMB B polarization to map the large-scale structures of the universe

Physical Review D

Volumn 63, Issue 4, 2001, Pages

  Benabed, K ^a,b   Bernardeau, F ^a,b   Van Waerbeke, L ^a,b  

^a CEA SACLAY   (France)

^b UNIVERSITY OF TORONTO   (Canada)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; COSMOS; GRAVITY; MATHEMATICAL ANALYSIS; MICROWAVE RADIATION; POLARIZATION; STATISTICAL ANALYSIS;

EID: 0035076493     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.63.043501     Document Type: Article

References (40)

1. Among the current and future high-precision observations, the most promising are probably the BOOMERanG balloon experiment. [B-. de Bernardis et al., New Astron. Rev. 43, 281 (1999)];
2. the MAP satellite mission [C.L. Bennett et al.. Am. Astron. Soc. Meeting 187, 7109 (1995)];
3. and Planck Surveyor satellite mission [M. Bersanelli et al., Report No. COBRAS/ SAMBA on the phase A study, ESA Report No. D/SCI(96)3].
4. M. Zaldarriaga, D. Spergel, and U. Seljak, Astrophys. J. 488, 1 (1997);
5. G. Efstathiou and J. R. Bond, Mon. Not. R. Astron. Soc. 304, 75 (1999).
6. S. Perlmutter et al, Astrophys. J. 517, 565 (1999);
7. A. G. Riess et al., Astron. J. 116, 1009 (1998).
8. A. Aguirre, Astrophys. J. 525, 583 (1999);
9. T. Totani and C. Kobayashi, Astrophys. J. Lett. 526, 65 (1999);
10. M. Livio, astro-ph/9903264;
11. K. Nomoto, astro-ph/9907386;
12. P. Valageas, Astron. Astrophys. 354, 767 (2000).
13. Y. Mellier, Annu. Rev. Astron. Astrophys. 37, 127 (1999).
14. A. Blanchard and J. Schneider, Astron. Astrophys. 184, 1 (1987);
15. U. Seljak, Astrophys. J. 463, 1 (1996).
16. F. Bernardeau, Astron. Astrophys. 324, 15 (1997);
17. M. Zaldar riaga, Phys. Rev. D 62, 063510 (2000).
18. F. Bernardeau, Astron. Astrophys. 338, 767 (1998).
19. U. Seljak and M. Zaldarriaga, Phys. Rev. Lett. 82, 2636 (1999);
20. M. Zaldarriaga and U. Seljak, Phys. Rev. D 58, 023003 (1998).
21. J. Guzik, U. Seljak, and M. Zaldarriaga, Phys. Rev. D 62, 043517 (2000).
22. M. Zaldarriaga and U. Seljak, Phys. Rev. D 58, 023003 (1998).
23. K. Benabed and F. Bernardeau, Phys. Rev. D 61, 123510 (2000).
24. M. Suginohara, T. Suginohara, and D. N. Spergel, Astrophys. J. 495, 511 (1998);
25. H. V. Peins and D. N. Spergel, ibid. 540, 605 (2000).
26. L. van Waerbeke, F. Bernardeau, and K. Benabed, Astrophys. J. 540, 14 (2000).
27. W. Hu, Phys. Rev. D 62, 043007 (2000).
28. V. Faraoni, Astron. Astrophys. 272, 385 (1993).
29. U. Seijak, Astrophys. J. 482, 6 (1997);
30. W. Hu and M. White, New Astron. 2, 323 (1997);
31. J. Lesgourgues, D. Polarski, S. Prunet, and A. A. Starobinsky, Astron. Astrophys. 359, 414 (2000).
32. A. Riazuelo, Ph.D. thesis, University of Paris 11, 2000.
33. L. van Waerbeke, F. Bernardeau, and Y. Mellier, astro-ph/9807007.
34. W. Hu, Astrophys. J. 529, 12 (2000).
35. F. R. Bouchet, S. Prunet, and S. K. Sethi, Mon. Not. R. Astron. Soc. 302, 663 (1999);
36. S. Prunet, S. K. Sethi, and F. R. Bouchet, Mon. Not. R. Astron. Soc. 314, 348 (2000).
37. J. A. Peacock and S. J. Dodds, Mon. Not. R. Astron. Soc. 280, L19 (1996).
38. F. Bernardeau, L. van Waerbeke, and Y. Mellier, Astron. Astrophys. 322, 1 (1997).
39. M. Srednicki, Astrophys. J. Lett. 416, 1 (1993).
40. B. Jain, U. Seijak, and S. White, Astrophys. J. 530, 547 (2000).