Large-scale nuclear structure calculations for spin-dependent WIMP scattering with chiral effective field theory currents

被引：174

作者：

Klos, P. ^{[1
,2
]}

Menendez, J. ^{[1
,2
]}

Gazit, D. ^{[3
,4
]}

Schwenk, A. ^{[1
,2
]}

机构：

[1] Tech Univ Darmstadt, Inst Kernphys, D-64289 Darmstadt, Germany

[2] GSI Helmholtzzentrum Schwerionenforschung GmbH, EMMI, D-64291 Darmstadt, Germany

[3] Hebrew Univ Jerusalem, Racah Inst Phys, IL-91904 Jerusalem, Israel

[4] Hebrew Univ Jerusalem, Ctr Nanosci & Nanotechnol, IL-91904 Jerusalem, Israel

来源：

PHYSICAL REVIEW D | 2013年 / 88卷 / 08期

关键词：

DARK-MATTER; SHELL-MODEL; CANDIDATES; PHYSICS; FORCES;

D O I：

10.1103/PhysRevD.88.083516

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We perform state-of-the-art large-scale shell-model calculations of the structure factors for elastic spin-dependent WIMP scattering off Xe-129,Xe-131, I-127, Ge-73, F-19, Na-23, Al-27, and Si-29. This comprehensive survey covers the nonzero-spin nuclei relevant to direct dark matter detection. We include a pedagogical presentation of the formalism necessary to describe elastic and inelastic WIMP-nucleus scattering. The valence spaces and nuclear interactions employed have been previously used in nuclear structure calculations for these mass regions and yield a good spectroscopic description of these isotopes. We use spin-dependent WIMP-nucleus currents based on chiral effective field theory at the one-body level and including the leading long-range two-body currents due to pion exchange, which are predicted in chiral effective field theory. Results for all structure factors are provided with theoretical error bands due to the nuclear uncertainties of WIMP currents in nuclei.

引用

页数：18

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