TL;DR
This paper calculates nuclear response functions for the Sun's elements to improve understanding of dark matter capture, revealing that momentum-dependent interactions can significantly influence capture rates and neutrino signals.
Contribution
It provides detailed nuclear response functions for 16 elements in the Sun and analyzes their impact on dark matter capture rates using effective theory.
Findings
Momentum-dependent couplings increase capture rates.
Different elements contribute variably to capture.
Response functions are provided in analytic form for future use.
Abstract
In the effective theory of isoscalar and isovector dark matter-nucleon interactions mediated by a heavy spin-1 or spin-0 particle, 8 isotope-dependent nuclear response functions can be generated in the dark matter scattering by nuclei. We compute the 8 nuclear response functions for the 16 most abundant elements in the Sun, i.e. H, He, He, C, N, O, Ne, Na, Mg, Al, Si, S, Ar, Ca, Fe, and Ni, through numerical shell model calculations. We use our response functions to compute the rate of dark matter capture by the Sun for all isoscalar and isovector dark matter-nucleon effective interactions, including several operators previously considered for dark matter direct detection only. We study in detail the dependence of the capture rate on specific dark matter-nucleon interaction operators,…
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