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Detecting domain walls of axionlike models using terrestrial experiments
M Pospelov1, S Pustelny, M P Ledbetter
1Department of Physics and Astronomy, University of Victoria, Victoria, British Columbia V8P 1A1, Canada.
Physical Review Letters
|February 7, 2013
Summary
Stable topological defects, like axionlike field domain walls, could explain dark energy and dark matter. Terrestrial experiments using synchronized atomic magnetometers show promise for detecting these phenomena and probing new physics.
Area of Science:
- Cosmology
- Particle Physics
- Astrophysics
Background:
- Stable topological defects from scalar fields may constitute dark energy and dark matter.
- Current constraints on these defects primarily come from gravitational and cosmological observations.
- Axionlike fields with spin couplings offer a specific model for generating domain walls.
Purpose of the Study:
- To investigate the feasibility of detecting domain walls generated by axionlike fields in galactic environments.
- To explore the potential of terrestrial experiments for probing unconstrained model parameters.
- To demonstrate the role of atomic magnetometers in detecting wall-crossing events.
Main Methods:
- Modeling domain walls formed by an axionlike field coupled to standard-model particle spins.
- Simulating the presence of a network of domain walls within the galactic environment.
- Proposing the use of a geographically separated, time-synchronized network of atomic magnetometers for detection.
Main Results:
- Terrestrial detection of wall-crossing events is shown to be realistic under specific galactic conditions.
- Atomic magnetometer networks can effectively detect these wall-crossing events.
- The proposed method can probe model parameters not currently constrained by astrophysical or gravitational experiments.
Conclusions:
- Terrestrial experiments offer a novel and realistic approach to detect topological defects.
- Atomic magnetometer networks provide a sensitive tool for exploring dark energy and dark matter candidates.
- This research opens new avenues for constraining axionlike field models and understanding the Universe's composition.
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