On the Rees-Sciama effect:: maps and statistics

被引：15

作者：

Puchades, N. ^{[1
]}

Fullana, M. J.

Arnau, J. V.

Saez, D.

机构：

[1] Univ Valencia, Dept Astron & Astrophys, E-46100 Burjassot, Spain

[2] Univ Politecn Valencia, Inst Matemat Multidisciplinar, E-46022 Valencia, Spain

[3] Univ Valencia, Dept Matemat Aplicada, E-46100 Burjassot, Spain

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2006年 / 370卷 / 04期

关键词：

methods : N-body simulations; methods : numerical; cosmic microwave background; cosmology theory; large-scale structure of Universe;

D O I：

10.1111/j.1365-2966.2006.10607.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Small maps of the Rees-Sciama (RS) effect are simulated by using an appropriate N-body code and a certain ray-tracing procedure. A method designed for the statistical analysis of cosmic microwave background (CMB) maps is applied to study the resulting simulations. These techniques, recently proposed - by our team - to consider lens deformations of the CMB, are adapted to deal with the RS effect. This effect and the deviations from Gaussianity associated to it seem to be too small to be detected in the near future. This conclusion follows from our estimation of both the RS angular power spectrum and the RS reduced n-direction correlation functions for n <= 6.

引用

页码：1849 / 1858

页数：10

共 35 条

[21] ANISOTROPIES IN THE MICROWAVE SKY DUE TO NONLINEAR STRUCTURES [J].

MARTINEZGONZALEZ, E ;

SANZ, JL ;

SILK, J .

ASTROPHYSICAL JOURNAL, 1990, 355 (01) :L5-L9

[22] CONTRIBUTION TO THE 3-POINT FUNCTION OF THE COSMIC MICROWAVE BACKGROUND FROM THE REES-SCIAMA EFFECT [J].

MOLLERACH, S ;

GANGUI, A ;

LUCCHIN, F ;

MATARRESE, S .

ASTROPHYSICAL JOURNAL, 1995, 453 (01) :1-5

[23] SKEWNESS OF COSMIC MICROWAVE BACKGROUND TEMPERATURE-FLUCTUATIONS DUE TO NONLINEAR GRAVITATIONAL-INSTABILITY [J].

MUNSHI, D ;

SOURADEEP, T ;

STAROBINSKY, AA .

ASTROPHYSICAL JOURNAL, 1995, 454 (02) :552-560

[24] First year Wilkinson Microwave Anisotropy Probe observations:: Dark energy induced correlation with radio sources [J].

Nolta, MR ;

Wright, EL ;

Page, L ;

Bennett, CL ;

Halpern, M ;

Hinshaw, G ;

Jarosik, N ;

Kogut, A ;

Limon, M ;

Meyer, SS ;

Spergel, DN ;

Tucker, GS ;

Wollack, E .

ASTROPHYSICAL JOURNAL, 2004, 608 (01) :10-15

[25] Correlating the CMB with luminous red galaxies: The integrated Sachs-Wolfe effect [J].

Padmanabhan, N ;

Hirata, CM ;

Seljak, U ;

Schlegel, DJ ;

Brinkmann, J ;

Schneider, DP .

PHYSICAL REVIEW D, 2005, 72 (04) :1-16

[26]

Peebles P. J. E., 1980, The large-scale structure of the universe, DOI DOI 10.23943/PRINCETON/9780691209838.001.0001

[27] On the role of shock waves in galaxy cluster evolution [J].

Quilis, V ;

Ibáñez, JM ;

Sáez, D .

ASTROPHYSICAL JOURNAL, 1998, 502 (02) :518-530

[28] Small angular scale simulations of the microwave sky [J].

Saez, D ;

Holtmann, E ;

Smoot, GF .

ASTROPHYSICAL JOURNAL, 1996, 473 (01) :1-6

[29] SAMPLE VARIANCE IN SMALL-SCALE COSMIC MICROWAVE BACKGROUND ANISOTROPY EXPERIMENTS [J].

SCOTT, D ;

SREDNICKI, M ;

WHITE, M .

ASTROPHYSICAL JOURNAL, 1994, 421 (01) :L5-U0007

[30] A line-of-sight integration approach to cosmic microwave background anisotropies [J].

Seljak, U ;

Zaldarriaga, M .

ASTROPHYSICAL JOURNAL, 1996, 469 (02) :437-444

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