2013
DOI: 10.1088/1475-7516/2013/10/019
|View full text |Cite
|
Sign up to set email alerts
|

Tools for model-independent bounds in direct dark matter searches

Abstract: We discuss a framework (based on non-relativistic operators) and a self-contained set of numerical tools to derive the bounds from some current direct detection experiments on virtually any arbitrary model of Dark Matter elastically scattering on nuclei.

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

4
385
1
1

Year Published

2014
2014
2022
2022

Publication Types

Select...
5
3

Relationship

1
7

Authors

Journals

citations
Cited by 271 publications
(391 citation statements)
references
References 64 publications
(128 reference statements)
4
385
1
1
Order By: Relevance
“…The computation is rather involved, due to subtle cancellations which occur between different operators (notably contributing to the 1-loop diagrams, which makes the inclusion of 2-loops necessary). It has been discussed over the years in [6,21,[68][69][70][71][72][73][74][75]. The most recent explicit computation, reported in [74] and based on [75], is performed in the framework of the 'heavy WIMP effective theory' and therefore assumes m W , m h M χ .…”
Section: Jhep10(2014)033mentioning
confidence: 99%
“…The computation is rather involved, due to subtle cancellations which occur between different operators (notably contributing to the 1-loop diagrams, which makes the inclusion of 2-loops necessary). It has been discussed over the years in [6,21,[68][69][70][71][72][73][74][75]. The most recent explicit computation, reported in [74] and based on [75], is performed in the framework of the 'heavy WIMP effective theory' and therefore assumes m W , m h M χ .…”
Section: Jhep10(2014)033mentioning
confidence: 99%
“…The couplings are determined in the standard way by embedding the quarks within the nucleon, as reviewed in ref. [49]:…”
Section: Jhep08(2016)111mentioning
confidence: 99%
“…[49]. 3 Calculation of the expected rate in the LUX experiment [58] is detailed in Addendum 1 of ref.…”
Section: Jhep08(2016)111mentioning
confidence: 99%
“…dominated by LUX data [48,50]. This bound assumes that techni-baryons constitute all galactic DM, and must be rescaled otherwise.…”
Section: Jhep01(2015)157mentioning
confidence: 99%
“…We thank Roberto Contino, Riccardo Rattazzi, Slava Rychkov, Riccardo Torre for advice about strong dynamics and the authors of [50] (in particular Eugenio del Nobile) for help about using their code. The work of OA and MR is supported by the MIUR-FIRB grant RBFR12H1MW.…”
Section: Acknowledgmentsmentioning
confidence: 99%