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1 vote
1 answer
183 views

Does NFW profile work for any galaxy?

We use Navarro–Frenk–White (NFW) to calculate Dark Matter (DM) density. Can we use it for DM halo in any galaxy or is it used only for Milky Way (MW)?
Peyman's user avatar
  • 11
3 votes
1 answer
119 views

Could a fourth family of quarks and leptons account for dark matter?

In the early universe, could a family of quarks and leptons have formed an electrically neutral particle that is dark matter?
user avatar
3 votes
0 answers
49 views

What properties of dark matter can we derive from each of the available methods for probing the physics of dark matter?

This is probably a long shot but it's worth trying. My question is the following: What properties of dark matter can we derive from each of the available methods for probing the physics of dark matter?...
Floyd's user avatar
  • 373
1 vote
0 answers
45 views

Possibility of reaching equilibrium starting with a nonequilibrium initial condition in the early radiation-domination

Update after @knzhou's comment If in a theory, the coupling of the dark matter (DM) field to the Standard Model (SM) fields is small enough, the rate of interaction of the DM particles in the ...
SRS's user avatar
  • 26.8k
1 vote
1 answer
192 views

Dark matter in the time window between freeze-out and kinetic decoupling

Background After the freeze-out, when all annihilations have stopped, the abundance ($Y=\frac{n}{s}$) of thermal dark matter species no longer changes with time. However, it is still kept in kinetic ...
SRS's user avatar
  • 26.8k
11 votes
2 answers
547 views

If neutrinos are disfavoured as DM candidates why aren't axions?

Numerical simulations of observed large-scale structure formation work best with Cold Dark Matter (CDM; see the answer here). Neutrinos are candidates for Hot Dark Matter (HDM), and hence they cannot ...
SRS's user avatar
  • 26.8k
3 votes
1 answer
1k views

Why is the dark matter freeze-out temperature $T\sim \frac{m}{20}$ so generic?

For a dark matter of mass $m$, the typical freeze-out temperature is $T$ is usually assumed to be between $\frac{m}{20}-\frac{m}{25}$. But the freeze-out temperature depends upon the annihilation ...
SRS's user avatar
  • 26.8k
0 votes
1 answer
186 views

Why can't the Higgs vacuum energy clump to galaxies and act as dark matter (instead of dark energy)? [closed]

The Higgs field has a nonzero vacuum expectation value which contributes to the energy density of the Universe. Energies contribute to the curvature of spacetime and affected by gravitational ...
SRS's user avatar
  • 26.8k
4 votes
1 answer
239 views

How are the dark matter (DM) thermalization rates derived in singlet DM model?

This well-cited paper talks about a minimal renormalizable extension to the Standard Model (SM) to incorporate particle dark matter (DM) into it by adding a real scalar field $S$ which (unlike the ...
SRS's user avatar
  • 26.8k
2 votes
2 answers
489 views

Why do we think that the dark sector is simpler?

Matter makes up roughly $5\%$ of the Universe while dark matter makes up roughly $25\%$. For matter and radiation, we have a complicated Standard model with many generations of fermions and various ...
SRS's user avatar
  • 26.8k
4 votes
1 answer
185 views

About the consequences of $\mathbb{Z}_2$ invariance in dark matter models

This well-cited paper talks about is a minimal renormalizable extension to the Standard Model (SM) to incorporate particle dark matter (DM) into it by adding a real scalar field $S$ which (unlike the ...
SRS's user avatar
  • 26.8k
5 votes
2 answers
190 views

Why did dark matter interact with the Standard model particles in the early Universe but not now?

In the thermal dark matter (DM) scenario, it is the interaction of the DM particles with the Standard Model (SM) particles that kept the DM particles in kinetic equilibrium with the thermal plasma. ...
SRS's user avatar
  • 26.8k
6 votes
1 answer
527 views

Why is the Standard model Higgs not a candidate of dark matter (in particular, a WIMP)?

Please consider me as a naive self-learner in this field. The Standard Model (SM) Higgs boson is electrically neutral and has a mass of around $125$ GeV (which lies in the WIMP window i.e., between ...
SRS's user avatar
  • 26.8k
4 votes
2 answers
183 views

What are the steps to identify a dark matter candidate?

By looking at the Lagrangian of a simple particle physics model, how do people identify the dark matter (DM) candidates, if any? One of the criteria is to check whether the electric charge of the ...
SRS's user avatar
  • 26.8k
3 votes
1 answer
249 views

How did dark matter become a relic?

Why did the decay rate of the dark matter particles fall when the temperature of the Universe $T_U$ dropped below dark matter mass $M_{DM}$? In particular, why can it not decay into lighter particles ...
SRS's user avatar
  • 26.8k

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