Longer Observation Times and Expanding the Mass Window
by Phenomenology TechnologyOctober 27th, 2024
Too Long; Didn't Read
Future dark matter detection efforts should focus on longer observation times and advanced detection methods, enabling the probing of higher mass ranges and accounting for Earth's rotational effects, thereby refining the signal analysis of vector dark matter signals.
Authors:
(1) Dorian W. P. Amaral, Department of Physics and Astronomy, Rice University and These authors contributed approximately equally to this work;
(2) Mudit Jain, Department of Physics and Astronomy, Rice University, Theoretical Particle Physics and Cosmology, King’s College London and These authors contributed approximately equally to this work;
(3) Mustafa A. Amin, Department of Physics and Astronomy, Rice University;
(4) Christopher Tunnell, Department of Physics and Astronomy, Rice University.
Table of Links
2 Calculating the Stochastic Wave Vector Dark Matter Signal
3 Statistical Analysis and 3.1 Signal Likelihood
4 Application to Accelerometer Studies
4.1 Recasting Generalised Limits onto B − L Dark Matter
6 Conclusions, Acknowledgments, and References
A Equipartition between Longitudinal and Transverse Modes
B Derivation of Marginal Likelihood with Stochastic Field Amplitude
D The Case of the Gradient of a Scalar
5 Future Directions
5.1 Longer Observation Times
5.2 Expanding the Mass Window
This paper is available on arxiv under CC BY 4.0 DEED license.
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