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Cosmic Matter Distribution: Cosmic Baryon Budget Revisited

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arxiv astro-ph/0312517 v1 pith:DNFE2DWC submitted 2003-12-19 astro-ph

classification astro-ph
keywords cosmicbaryonbudgetrevisitedabundanceaccountingaccuracyamount
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abstract

The cosmic baryon budget is revisited using modern observations that have become available since our first publication. I also present an estimate for the heavy element abundance. An increased accuracy in the accounting of the baryon budget reveals `missing baryons', which amount to $\approx 35$% of the total. This would provide an interesting test for models of the cosmic structure formation.

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Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Tracing cosmic gas in filaments and halos: Low-redshift insights from the kinematic Sunyaev-Zel'dovich effect

    astro-ph.CO 2024-12 conditional novelty 7.0 of 10

    A 4-sigma kinematic Sunyaev-Zel'dovich quadrupole detection shows gas around low-redshift galaxy groups is aligned with cosmic filaments, the first such kSZ measurement.

  2. Picolensing as a Probe of Primordial Black Hole Dark Matter

    astro-ph.HE 2024-11 conditional novelty 5.0 of 10

    Asteroid-mass primordial black hole dark matter could be probed by picolensing of gamma-ray bursts, but only with detector separations of at least Earth-L2 distance once realistic GRB size uncertainties are included.

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