Looking at cosmic near-infrared background radiation anisotropies

被引：59

作者：

Kashlinsky, A. ^{[1
,2
]}

Arendt, R. G. ^{[1
,3
]}

Atrio-Barandela, F. ^{[4
]}

Cappelluti, N. ^{[5
,6
]}

Ferrara, A. ^{[7
]}

Hasinger, G. ^{[8
]}

机构：

[1] Goddard Space Flight Ctr, Observat Cosmol Lab, Code 665, Greenbelt, MD 20771 USA

[2] SSAI, Lanham, MD 20706 USA

[3] Univ Maryland, CRESST, Baltimore, MD 21250 USA

[4] Univ Salamanca, Dept Fundamental Phys, Salamanca 37008, Spain

[5] Yale Ctr Astron & Astrophys, POB 208120, New Haven, CT 06520 USA

[6] Univ Miami, Dept Phys, Coral Gables, FL 33124 USA

[7] Scuola Normale Super Pisa, Piazza Cavalieri 7, I-56126 Pisa, Italy

[8] Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA

来源：

REVIEWS OF MODERN PHYSICS | 2018年 / 90卷 / 02期

关键词：

SUPERMASSIVE BLACK-HOLES; POPULATION-III STARS; ULTRA DEEP FIELD; COBE DIRBE MAPS; SMALL-SCALE FLUCTUATIONS; ACTIVE GALACTIC NUCLEUS; PROBE WMAP OBSERVATIONS; INITIAL MASS FUNCTION; BILLION YEARS PROJECT; DARK-MATTER HALOES;

D O I：

10.1103/RevModPhys.90.025006

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The cosmic infrared background (CIB) contains emissions accumulated over the entire history of the Universe, including from objects inaccessible to individual telescopic studies. The near-infrared (similar to 1-10 pm) part of the CIB, and its fluctuations, reflects emissions from nucleosynthetic sources and gravitationally accreting black holes. If known galaxies are removed to sufficient depths the source-subtracted CIB fluctuations at near-infrared can reveal sources present in the first stars era and possibly new stellar populations at more recent times. This review discusses the recent progress in this newly emerging field which identified, with new data and methodology, significant source-subtracted CIB fluctuations substantially in excess of what can be produced by remaining known galaxies. The CIB fluctuations further appear coherent with unresolved cosmic x-ray background indicating a very high fraction of black holes among the new sources producing the CIB fluctuations. These observations have led to intensive theoretical efforts to explain the measurements and their properties. While current experimental configurations have limitations in decisively probing these theories, their potentially remarkable implications will be tested in the upcoming CD3 measurements with the European Space Agency's Euclid dark energy mission. The goals and methodologies of L[BRAE (Looking at Infrared Background Radiation with Euclid), a National Aeronautics and Space Administration (NASA) selected project for CIB science with Euclid, which has the potential for transforming the field into a new area of precision cosmology, are described.

引用

页数：57

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