Numerical Simulations Unravel the Cosmic Web

The universe is permeated by a network of filaments, sheets, and knots collectively forming a “cosmic web.” The discovery of the cosmic web, especially through its signature of absorption of light from distant sources by neutral hydrogen in the intervening intergalactic medium, exemplifies the interplay between theory and experiment that drives science and is one of the great examples in which numerical simulations have played a key and decisive role. We recount the milestones in our understanding of cosmic structure; summarize its impact on astronomy, cosmology, and physics; and look ahead by outlining the challenges faced as we prepare to probe the cosmic web at new wavelengths.

[1]  J. Bond,et al.  How filaments of galaxies are woven into the cosmic web , 1995, Nature.

[2]  Rupert A. C. Croft,et al.  Recovery of the Power Spectrum of Mass Fluctuations from Observations of the Lyα Forest , 1998 .

[3]  Bruce A. Peterson,et al.  On the Density of Neutral Hydrogen in Intergalactic Space , 1965 .

[4]  THE LYMAN ALPHA FOREST IN THE SPECTRA OF QUASISTELLAR OBJECTS , 1998, astro-ph/9806286.

[5]  D. Weinberg,et al.  Baryons in the Warm-Hot Intergalactic Medium , 2000, astro-ph/0007217.

[6]  H. Trac,et al.  Can sterile neutrinos be the dark matter? , 2006, Physical review letters.

[7]  P. Scheuer A Sensitive Test for the Presence of Atomic Hydrogen in Intergalactic Space , 1965, Nature.

[8]  J. Ostriker,et al.  Physical properties of the intergalactic medium and the Lyman-alpha absorbing clouds , 1983 .

[9]  Edward J. Wollack,et al.  First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Determination of cosmological parameters , 2003, astro-ph/0302209.

[10]  Geoffrey Burbidge,et al.  On the measurement and interpretation of absorption features in the spectrum of the quasi-stellar object 3C 191. , 1966 .

[11]  G. Hinshaw,et al.  Structure in the COBE differential microwave radiometer first-year maps , 1992 .

[12]  Maarten Schmidt,et al.  LARGE REDSHIFTS OF FIVE QUASI-STELLAR SOURCES , 1965 .

[13]  The morphology of H ii regions during reionization , 2006, astro-ph/0610094.

[14]  John N. Bahcall,et al.  On the interaction of radiation from distant sources with the intervening medium. , 1965 .

[15]  L. Hernquist,et al.  The Opacity of the Lyα Forest and Implications for Ωb and the Ionizing Background , 1996, astro-ph/9612245.

[16]  J. Lesgourgues,et al.  Can sterile neutrinos be ruled out as warm dark matter candidates? , 2006, Physical review letters.

[17]  Matias Zaldarriaga,et al.  Simulations and Analytic Calculations of Bubble Growth during Hydrogen Reionization , 2006, astro-ph/0604177.

[18]  J. Brinkmann,et al.  The Linear Theory Power Spectrum from the Lyα Forest in the Sloan Digital Sky Survey , 2004, astro-ph/0407377.

[19]  Simon D. M. White,et al.  Clustering in a neutrino-dominated universe , 1983 .

[20]  October I Physical Review Letters , 2022 .

[21]  A. Boksenberg,et al.  The distribution of Lyman-alpha absorption lines in the spectra of six QSOs: evidence for an intergalactic origin. , 1980 .

[22]  R. Cen,et al.  Where Are the Baryons , 1998, astro-ph/9806281.

[23]  P. Peebles,et al.  STATISTICAL TESTS FOR THE ORIGIN OF ABSORPTION LINES OBSERVED IN QUASI- STELLAR SOURCES. , 1969 .

[24]  R. Rosenfeld Nature , 2009, Otolaryngology--head and neck surgery : official journal of American Academy of Otolaryngology-Head and Neck Surgery.