Fluctuations in the cosmic microwave background. II. Cl at large and small l

Physical Review D

Volumn 64, Issue 12, 2001, Pages

  Weinberg, Steven ^a  

^a UNIVERSITY OF TEXAS AT AUSTIN   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ACCURACY; ACOUSTICS; ARTICLE; CALCULATION; COSMIC RADIATION; COSMOS; DIPOLE; DOPPLER FLOWMETRY; MATHEMATICAL ANALYSIS; MICROWAVE RADIATION; MODEL; OSCILLATION; TEMPERATURE;

EID: 0035893640     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.64.123512     Document Type: Article

References (8)

1. S. Weinberg, preceding paper, Phys. Rev. D 64, 123511 (2001).
2. L.P. Grishchuk and J. Martin, Phys. Rev. D 56, 1924 (1997).
3. J. R. Bond, in Cosmology and Large Scale Structure, edited by R. Schaeffer, J. Silk, M. Spiro, and J. Zinn-Justin (Elsevier, Amsterdam, 1996), Section 5.1.3. Our result (26) can also be derived with somewhat more trouble by using Bond's results on the asymptotic behavior of averaged products of spherical Bessel functions.
4. This method had been used previously to obtain Eq. (21) with only a scalar form-factor F(k), as, for instance, by J.R. Bond and G. Efstathiou, Mon. Not. R. Astron. Soc. 226, 655 (1987), Eq. (4.19), but not as far as I know with the inclusion of the dipole form-factor G(k).
5. I. S. Gradshteyn and I. M. Ryzhik, Table of Integrals, Series, and Products (Academic Press, New York, 1980), no. 6.671.2.
6. Gradshteyn and Ryzhik [5], no. 6.574.2.
7. G. 't Hooft and M. Veltman, Nucl. Phys. B44, 189 (1972).
8. E.F. Bunn and M. White, Astrophys. J. 480, 6 (1997).