The effect of reionization on the COBE normalization

被引:6
作者
Griffiths, LM
Liddle, AR
机构
[1] Astrophys Nucl & Astrophys Lab, Oxford OX1 3RH, England
[2] Univ Sussex, Ctr Astron, Brighton BN1 9QJ, E Sussex, England
关键词
cosmic microwave background; cosmology : theory;
D O I
10.1046/j.1365-8711.2001.04403.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We point out that the effect of reionization on the microwave anisotropy power spectrum is not necessarily negligible on the scales probed by COBE. It can lead to an upward shift of the COBE normalization by more than the 1 sigma error quoted, ignoring reionization. We provide a fitting function to incorporate reionization into the normalization of the matter power spectrum.
引用
收藏
页码:769 / 771
页数:3
相关论文
共 15 条
[1]   Four-year COBE DMR cosmic microwave background observations: Maps and basic results [J].
Bennett, CL ;
Banday, AJ ;
Gorski, KM ;
Hinshaw, G ;
Jackson, P ;
Keegstra, P ;
Kogut, A ;
Smoot, GF ;
Wilkinson, DT ;
Wright, EL .
ASTROPHYSICAL JOURNAL, 1996, 464 (01) :L1-&
[2]   Four-year COBE normalization of inflationary cosmologies [J].
Bunn, EF ;
Liddle, AR ;
White, M .
PHYSICAL REVIEW D, 1996, 54 (10) :R5917-R5921
[3]   The 4 year COBE normalization and large-scale structure [J].
Bunn, EF ;
White, M .
ASTROPHYSICAL JOURNAL, 1997, 480 (01) :6-21
[4]   Cosmic microwave background constraints on the epoch of reionization [J].
Griffiths, LM ;
Barbosa, D ;
Liddle, AR .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1999, 308 (03) :854-862
[5]   ON DENSITY OF NEUTRAL HYDROGEN IN INTERGALACTIC SPACE [J].
GUNN, JE ;
PETERSON, BA .
ASTROPHYSICAL JOURNAL, 1965, 142 (04) :1633-&
[6]  
Haiman Z, 1999, ASTR SOC P, V181, P227
[7]   The damping tail of cosmic microwave background anisotropies [J].
Hu, W ;
White, M .
ASTROPHYSICAL JOURNAL, 1997, 479 (02) :568-579
[8]   Cosmology from MAXIMA-1, BOOMERANG, and COBE DMR cosmic microwave background observations [J].
Jaffe, AH ;
Ade, PAR ;
Balbi, A ;
Bock, JJ ;
Bond, JR ;
Borrill, J ;
Boscaleri, A ;
Coble, K ;
Crill, BP ;
de Bernardis, P ;
Farese, P ;
Ferreira, PG ;
Ganga, K ;
Giacometti, M ;
Hanany, S ;
Hivon, E ;
Hristov, VV ;
Iacoangeli, A ;
Lange, AE ;
Lee, AT ;
Martinis, L ;
Masi, S ;
Mauskopf, PD ;
Melchiorri, A ;
Montroy, T ;
Netterfield, CB ;
Oh, S ;
Pascale, E ;
Piacentini, F ;
Pogosyan, D ;
Prunet, S ;
Rabii, B ;
Rao, S ;
Richards, PL ;
Romeo, G ;
Ruhl, JE ;
Scaramuzzi, F ;
Sforna, D ;
Smoot, GF ;
Stompor, R ;
Winant, CD ;
Wu, JHP .
PHYSICAL REVIEW LETTERS, 2001, 86 (16) :3475-3479
[9]   Efficient computation of cosmic microwave background anisotropies in closed Friedmann-Robertson-Walker models [J].
Lewis, A ;
Challinor, A ;
Lasenby, A .
ASTROPHYSICAL JOURNAL, 2000, 538 (02) :473-476
[10]   How exactly did the universe become neutral? [J].
Seager, S ;
Sasselov, DD ;
Scott, D .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2000, 128 (02) :407-430