Shell Model Description of Spin-Dependent Elastic and Inelastic WIMP Scattering off <sup>119</sup>Sn and <sup>121</sup>Sb

In this work, we calculate the spin structure functions for spin-dependent elastic and inelastic WIMP scattering off <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msup><mrow></mrow><mn>119&l...

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Main Authors: Joona Kasurinen, Jouni Suhonen, Praveen C. Srivastava, Pekka Pirinen
Format: Article
Language:English
Published: MDPI AG 2022-05-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/8/6/309
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author Joona Kasurinen
Jouni Suhonen
Praveen C. Srivastava
Pekka Pirinen
author_facet Joona Kasurinen
Jouni Suhonen
Praveen C. Srivastava
Pekka Pirinen
author_sort Joona Kasurinen
collection DOAJ
description In this work, we calculate the spin structure functions for spin-dependent elastic and inelastic WIMP scattering off <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msup><mrow></mrow><mn>119</mn></msup></semantics></math></inline-formula>Sn and <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msup><mrow></mrow><mn>121</mn></msup></semantics></math></inline-formula>Sb. Estimates for detection rates are also given. <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msup><mrow></mrow><mn>119</mn></msup></semantics></math></inline-formula>Sn and <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msup><mrow></mrow><mn>121</mn></msup></semantics></math></inline-formula>Sb are amenable to nuclear structure calculations using the nuclear shell model (NSM). With the possible exception of <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msup><mrow></mrow><mn>201</mn></msup></semantics></math></inline-formula>Hg, they are the only such nuclei still unexplored theoretically for their potential of inelastic WIMP scattering to a very low excited state. The present calculations were conducted using a state-of-the-art WIMP–nucleus scattering formalism, and the available effective NSM two-body interactions describe the spectroscopic properties of these nuclei reasonably well. Structure functions were found to be high for both nuclei in the case of elastic scattering. Elastic scattering dominated at the zero momentum transfer limit. Detection rate calculations indicated that inelastic scattering was relevant for both nuclei, even surpassing elastic rates for some recoil energies.
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spelling doaj.art-587cfb5accce4f68b877e15acf44be172023-11-23T19:19:04ZengMDPI AGUniverse2218-19972022-05-018630910.3390/universe8060309Shell Model Description of Spin-Dependent Elastic and Inelastic WIMP Scattering off <sup>119</sup>Sn and <sup>121</sup>SbJoona Kasurinen0Jouni Suhonen1Praveen C. Srivastava2Pekka Pirinen3Department of Physics, University of Jyväskylä, P.O. Box 35 (YFL), 40014 Jyväskylä, FinlandDepartment of Physics, University of Jyväskylä, P.O. Box 35 (YFL), 40014 Jyväskylä, FinlandDepartment of Physics, Indian Institute of Technology Roorkee, Roorkee 247667, IndiaDepartment of Physics, University of Jyväskylä, P.O. Box 35 (YFL), 40014 Jyväskylä, FinlandIn this work, we calculate the spin structure functions for spin-dependent elastic and inelastic WIMP scattering off <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msup><mrow></mrow><mn>119</mn></msup></semantics></math></inline-formula>Sn and <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msup><mrow></mrow><mn>121</mn></msup></semantics></math></inline-formula>Sb. Estimates for detection rates are also given. <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msup><mrow></mrow><mn>119</mn></msup></semantics></math></inline-formula>Sn and <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msup><mrow></mrow><mn>121</mn></msup></semantics></math></inline-formula>Sb are amenable to nuclear structure calculations using the nuclear shell model (NSM). With the possible exception of <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msup><mrow></mrow><mn>201</mn></msup></semantics></math></inline-formula>Hg, they are the only such nuclei still unexplored theoretically for their potential of inelastic WIMP scattering to a very low excited state. The present calculations were conducted using a state-of-the-art WIMP–nucleus scattering formalism, and the available effective NSM two-body interactions describe the spectroscopic properties of these nuclei reasonably well. Structure functions were found to be high for both nuclei in the case of elastic scattering. Elastic scattering dominated at the zero momentum transfer limit. Detection rate calculations indicated that inelastic scattering was relevant for both nuclei, even surpassing elastic rates for some recoil energies.https://www.mdpi.com/2218-1997/8/6/309dark matterWIMPdirect detectionspin structure functionsnuclear structure
spellingShingle Joona Kasurinen
Jouni Suhonen
Praveen C. Srivastava
Pekka Pirinen
Shell Model Description of Spin-Dependent Elastic and Inelastic WIMP Scattering off <sup>119</sup>Sn and <sup>121</sup>Sb
Universe
dark matter
WIMP
direct detection
spin structure functions
nuclear structure
title Shell Model Description of Spin-Dependent Elastic and Inelastic WIMP Scattering off <sup>119</sup>Sn and <sup>121</sup>Sb
title_full Shell Model Description of Spin-Dependent Elastic and Inelastic WIMP Scattering off <sup>119</sup>Sn and <sup>121</sup>Sb
title_fullStr Shell Model Description of Spin-Dependent Elastic and Inelastic WIMP Scattering off <sup>119</sup>Sn and <sup>121</sup>Sb
title_full_unstemmed Shell Model Description of Spin-Dependent Elastic and Inelastic WIMP Scattering off <sup>119</sup>Sn and <sup>121</sup>Sb
title_short Shell Model Description of Spin-Dependent Elastic and Inelastic WIMP Scattering off <sup>119</sup>Sn and <sup>121</sup>Sb
title_sort shell model description of spin dependent elastic and inelastic wimp scattering off sup 119 sup sn and sup 121 sup sb
topic dark matter
WIMP
direct detection
spin structure functions
nuclear structure
url https://www.mdpi.com/2218-1997/8/6/309
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AT jounisuhonen shellmodeldescriptionofspindependentelasticandinelasticwimpscatteringoffsup119supsnandsup121supsb
AT praveencsrivastava shellmodeldescriptionofspindependentelasticandinelasticwimpscatteringoffsup119supsnandsup121supsb
AT pekkapirinen shellmodeldescriptionofspindependentelasticandinelasticwimpscatteringoffsup119supsnandsup121supsb