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Sub-GeV dark matter in superfluid He-4: an effective theory approach
Francesca Acanfora1, Angelo Esposito2, Antonio D Polosa3
11Dipartimento di Fisica, Sapienza Università di Roma, P.le A Moro 2, Rome, 00185 Italy.
This study explores detecting sub-GeV dark matter by analyzing its interactions with superfluid Helium-4 phonons. Combined phonon emission rates create a significant exclusion region for dark matter mass, advancing dark matter detection strategies.
Area of Science:
- Particle Physics
- Condensed Matter Physics
- Cosmology
Background:
- Dark matter remains undetected, necessitating novel detection strategies.
- Superfluid Helium-4 possesses unique gapless excitations (phonons) interacting with potential dark matter candidates.
Purpose of the Study:
- Investigate the detectability of sub-GeV dark matter via interactions with superfluid Helium-4 phonons.
- Utilize effective field theory and symmetry principles to model dark matter-phonon interactions.
Main Methods:
- Employ an effective field theory framework to describe dark matter interactions.
- Calculate emission rates for one and two phonons.
- Analyze differential distributions for phonon excitations.
Main Results:
- Symmetry dictates the possible interactions between dark matter and superfluid phonons.
- Combined analysis of one- and two-phonon emission provides a substantial exclusion region for dark matter masses.
- The effective field theory is well-defined for softer phonon excitations.
Conclusions:
- The proposed method offers a viable approach for constraining sub-GeV dark matter models.
- The framework is extensible to various dark matter models and detection scenarios.
- This research enhances strategies for direct dark matter detection experiments.
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