Effective theory approach to direct detection of dark matter

Junji Hisano

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Effective theory approach to direct detection of dark matter

Junji Hisano

High Energy Physics - Phenomenology · Submitted 8 Dec 2017

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim An effective field theory approach is presented for evaluation of the dark matter direct detection rate in this lecture note.

how it is stated · asserted 0.99 read the record →

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The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

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Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 2,226 input tokens.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.08 · human participants 0.02 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.03 · compares with prior results 0.04 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v2. Results and the main claim are underlined; show every role.

An effective field theory approach is presented for evaluation of the dark matter direct detection rate in this lecture note. This is prepared for the Les Houches Summer School Effective Field Theory in Particle Physics and Cosmology, July 2017.

background contribution method result interpretation main claim

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#	sentence	role	the authors' own work	states the main conclusion	strength
s0	An effective field theory approach is presented for evaluation of the dark matter direct detection rate in this lecture note.	contribution 0.88	0.67	0.20	asserted 0.99
s1	This is prepared for the Les Houches Summer School Effective Field Theory in Particle Physics and Cosmology, July 2017.	background 0.98	0.31	0.02	asserted 0.96

What kind of paper the classifier reports this is: method or tool 0.77 · evidence from proof or derivation 0.79.

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The paper

Original abstract

An effective field theory approach is presented for evaluation of the dark matter direct detection rate in this lecture note. This is prepared for the Les Houches Summer School Effective Field Theory in Particle Physics and Cosmology, July 2017.

Human review

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References

Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

Light top-flavoured dark matter in dark SMEFT: one-loop matching and phenomenology
hep-ph 2026-10 accept novelty 6.0 of 10

In dark SMEFT, one-loop matching of top-flavoured dark matter shows that only tree-level operators can explain the Belle II B+→K+ννbar excess with O(1) couplings at Λ=1 TeV, with B0→K*0+inv giving the strongest constraint.
Spin-independent scattering of pseudoscalar-mediated dark matter
hep-ph 2026-09 accept novelty 6.0 of 10

Loop-induced spin-independent dark matter scattering from a pseudoscalar mediator can exceed the neutrino floor only if new physics appears below the TeV scale.
Loop corrections to dark matter direct detection in a pseudoscalar mediator dark matter model
hep-ph 2018-10 accept novelty 6.0 of 10

A corrected two-loop evaluation of the DM-gluon operator, plus previously omitted Higgs-portal quartic couplings, changes the predicted spin-independent cross section in pseudoscalar-mediator dark matter and lets a no...

How the literature uses it

13 arXiv papers cite this in 19 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

Papers citing it · 10 sentences without a confident label

Uses its method or tool 5 papers

If DM is a Majorana fermion, the relevant effective operators for the evaluation of the DM-nucleon SI scattering cross section are given by [equation] where $O _ μν^q$ is the twist-2 operator for quark $q$, [equation] We use the following relations to evaluate the SI cross section from these operators [ref] , [equation] where $N$ stands for a nucleon ($p$, $n$), and $m_N$ is its mass.

Loop corrections to dark matter direct detection in a pseudoscalar mediator dark matter model · Direct Detection · 0.89
Following Refs. [ref] , we calculate Wilson coefficients of the scalar-type and twist-2 DM-bottom-quark effective operators which arise from the box and triangle diagrams, as well as Wilson coefficient of DM-gluon effective operator [ref] which arises at the two-loop level.

Probing Bottom-flavored Scalar Dark Matters at Loop Level · Introduction · 0.94
We calculate effective operators for the evaluation of MDM-nucleon spin independent scattering cross section following [ref] .

Direct detections of Majorana dark matter in vector portal · Introduction · 0.99

Uses its data or values 1 paper

Values of $f_T_q^N$ can be found in [ref] .

Dark Matter from a Conformal Dark Sector · $T <$ (MS, HB, RGB) · 1.00

Cites it as background 2 papers

The matrix element of the scalar heavy quark density between nucleon states is a relevant contribution to the cross-section for the scalar interaction of dark matter with ordinary matter [ref] .

How perturbative are heavy sea quarks? · Heavy quark content of the nucleon · 0.80
Hadron-level interactions can induce either elastic or inelastic scattering of the DM off a nuclear target, depending on the model of the dark sector [ref] .

Constraining Gluonic Contact Interaction of a Neutrino-philic Dark Fermion at Hadron Colliders and Direct Detection Experiments · Absorption at Nuclear Targets · 0.88

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