Synopsis: Tackling the Small-Scale Crisis

Precise measurement of the cosmic microwave background could solve a problem of current cosmological models known as the small-scale crisis.
Synopsis figure
ESA/Hubble

The current paradigm for describing cosmological evolution, known as the Λ CDM model, successfully explains the large-scale structure of the Universe—the organization of galaxies into clusters, sheets, or filaments separated by giant voids. However, Λ CDM predicts more small-scale structures, such as dwarf galaxies, than are actually present—a problem called the "small scale crisis." Tomohiro Nakama of Johns Hopkins University, Maryland, and colleagues now suggest that measurements of the spectrum of the cosmic microwave background (CMB) could shed light on the causes of the small-scale crisis.

The structures in the present Universe derive from density fluctuations in the early Universe. The dearth of small-scale structures may imply that some exotic mechanisms suppressed such fluctuations on small length scales. These mechanisms could be primordial, related to unknown processes occurring during cosmic inflation in the very early Universe. Alternatively, density-fluctuation suppression may have happened later, possibly caused by warm forms of dark matter or by the interaction of dark matter with visible matter.

Nakama and his co-workers argue that early- and late-time suppression mechanisms could, in principle, be distinguished through precise measurement of the CMB’s frequency spectrum. This spectrum is extremely close to that of an ideal blackbody. However, suppression of density fluctuations would cause spectral distortions, characterizable through a “chemical potential” called 𝜇. According to the team’s calculations, 𝜇 would be very small or negative for primordial suppression, while it would have larger positive values for late-time suppression.

This research is published in Physical Review D.

–Matteo Rini

Matteo Rini is the Deputy Editor of Physics.


Features

More Features »

Announcements

More Announcements »

Subject Areas

CosmologyAstrophysics

Previous Synopsis

Graphene

Crumpled Graphene

Read More »

Next Synopsis

Atomic and Molecular Physics

Tracking a Trapped Ion Crystal

Read More »

Related Articles

Synopsis: Self-Interacting Dark Matter Scores Again
Cosmology

Synopsis: Self-Interacting Dark Matter Scores Again

Dark matter that interacts with itself provides a better description of the speeds of stars in galaxies than dark matter that doesn’t self-interact. Read More »

Synopsis: Searching for Neutron Star Gravitational Waves
Astrophysics

Synopsis: Searching for Neutron Star Gravitational Waves

The first run of LIGO and Virgo’s gravitational-wave search shows no evidence of spinning asymmetric neutron stars, but recent upgrades could make the detection possible. Read More »

Viewpoint: Neutron-Star Implosions as Heavy-Element Sources
Cosmology

Viewpoint: Neutron-Star Implosions as Heavy-Element Sources

A dramatic scenario in which a compact black hole eats a spinning neutron star from inside might explain a nearby galaxy’s unexpectedly high abundance of heavy elements. Read More »

More Articles