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Cooling an Optically Trapped Ultracold Fermi Gas by Periodical Driving
Published on: March 30, 2017
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Cosmology of Sub-MeV Dark Matter Freeze-In.
Cora Dvorkin1, Tongyan Lin2, Katelin Schutz3,4
1Department of Physics, Harvard University, Cambridge, Massachusetts 02138, USA.
Physical Review Letters
|September 24, 2021
Summary
This study explores freeze-in dark matter (DM) produced via a light mediator. Combining cosmological data, we constrain DM masses up to 20 keV and forecast future explorations up to 80 keV.
Area of Science:
- Cosmology
- Particle Physics
- Astrophysics
Background:
- Dark matter (DM) is a significant component of the universe, but its nature remains unknown.
- Freeze-in production offers a viable mechanism for generating DM through feeble interactions in the early universe.
- Light DM candidates with effective electric charges can impact cosmological evolution.
Purpose of the Study:
- To constrain the mass of freeze-in dark matter using a combination of observational data.
- To forecast the potential of future experiments in probing higher mass ranges for freeze-in DM.
- To investigate the observable consequences of DM produced via freeze-in in the standard model plasma.
Main Methods:
- Utilizing data from the cosmic microwave background (CMB).
- Analyzing Lyman-α forest, quasar lensing, stellar streams, and Milky Way satellite abundances.
- Performing forecasts for upcoming experiments like CMB-S4, HERA, and the Vera Rubin Observatory.
Main Results:
- Setting limits on freeze-in dark matter masses up to approximately 20 keV.
- The exact constraint depends on whether the dark matter thermalizes within its own sector.
- Forecasting the exploration of freeze-in dark matter masses up to approximately 80 keV with future experiments.
Conclusions:
- Freeze-in dark matter with a light mediator is a plausible scenario.
- Current cosmological and astrophysical data provide significant constraints on freeze-in DM properties.
- Future observational facilities will greatly enhance our ability to detect and characterize freeze-in dark matter.
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