Velocity independent constraints on spin-dependent DM-nucleon interactions from IceCube and PICO

Velocity independent constraints on spin-dependent DM-nucleon interactions from IceCube and PICO

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Abstract Adopting the Standard Halo Model (SHM) of an isotropic Maxwellian velocity distribution for dark matter (DM) particles in the Galaxy, the most stringent current constraints on their spin-dependent scattering cross-section with nucleons come from the IceCube neutrino observatory and the PIC...

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Bibliographic Details
Main Authors: Aartsen, M. G, Ackermann, M., Adams, J., Aguilar, J. A, Ahlers, M., Ahrens, M., Alispach, C., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Argüelles, C., Auffenberg, J., Axani, S., Backes, P., Bagherpour, H., Bai, X., Balagopal V., A., Barbano, A., Barwick, S. W
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:English
Published: Springer Berlin Heidelberg 2021
Online Access:https://hdl.handle.net/1721.1/131292

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https://hdl.handle.net/1721.1/131292

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