{"arxiv_id":"hep-ph/0207125","incoming":{"papers":122,"sentences":156,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":4,"sentences":6,"quotes":[{"arxiv_id":"1910.02322","title":"Addressing $\\gamma$-ray emissions from dark matter annihilations in 45 milky way satellite galaxies and in extragalactic sources with particle dark matter models","url":"/paper/1910.02322","section":"Formalism for $γ$-ray flux calculations in case of dwarf galaxies from dark matter annihilation","sentence":"For the case of $B^1$ dark matter, the annihilation cross-section $B^1 B^1 ⟶qq$ is computed from the expression [ref] [equation] where $q_L^1$ is the first KK partner of the quark $q_L$, $Y_q_L^1$ and $m_q_L^1$ are respectively the corresponding hypercharge and mass while $θ_W$ is the Weinberg angle.","intent_p":0.92,"contests_p":null},{"arxiv_id":"2102.00959","title":"Bounds on abundance of primordial black hole and dark matter from EDGES 21-cm signal","url":"/paper/2102.00959","section":"Introduction","sentence":"Throughout the calculation, the baryon-DM interaction cross-section ($σ̅$) is parameterized as $σ̅=σ_0 v^-4$ [ref] , where the considered dark matter is assumed to be model-independent [ref] .","intent_p":0.86,"contests_p":null},{"arxiv_id":"0705.2502","title":"WIMP identification through a combined measurement of axial and scalar couplings","url":"/paper/0705.2502","section":"Introduction","sentence":"Our calculation of the LKP scattering cross section off nucleons closely follows [ref] (see also [ref] ).","intent_p":1.0,"contests_p":null},{"arxiv_id":"0805.4210","title":"Kaluza-Klein Dark Matter: Direct Detection vis-a-vis LHC","url":"/paper/0805.4210","section":"Elastic Scattering Cross Sections","sentence":"We follow the computation done in [ref] [The precise calculation of the heavy quark contribution to the processes of Fig. [ref] is rather involved – the heavy flavors contribute only at the loop level, through the gluon content of the nucleon.","intent_p":0.81,"contests_p":null}]},{"kind":"comparison","label":"Compares with it","papers":6,"sentences":6,"quotes":[{"arxiv_id":"1509.03683","title":"MadDM: New Dark Matter Tool in the LHC era","url":"/paper/1509.03683","section":"MadDM and Validation","sentence":"For MUED, Fig. [ref] shows excellent agreement between MadDM cross sections and results in literature [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"1505.04190","title":"Direct Detection of Dark Matter with MadDM v.2.0","url":"/paper/1505.04190","section":"Minimal Universal Extra Dimensions","sentence":"We compared the results against those using the private code used in Refs. [ref] .","intent_p":0.98,"contests_p":null},{"arxiv_id":"0803.0631","title":"Photons from Dark Matter in a (non-Universal) Extra Dimension model","url":"/paper/0803.0631","section":"Introduction","sentence":"From the point of view of indirect searches, this feature distinguishes $A_-$ from the UED WIMP candidate $B^1$ [ref] , whose pairs annihilation branching ratios are dominated by charged leptons and harder spectra are produced.","intent_p":0.98,"contests_p":null},{"arxiv_id":"1310.8621","title":"Dark Matter in the Coming Decade: Complementary Paths to Discovery and Beyond","url":"/paper/1310.8621","section":"Universal Extra Dimensions","sentence":"In Fig. [ref] we contrast the LHC reach with the relic density constraints [ref] and with the sensitivity of direct detection experiments [ref] .","intent_p":0.86,"contests_p":null},{"arxiv_id":"0706.3409","title":"Spinless photon dark matter from two universal extra dimensions","url":"/paper/0706.3409","section":"Direct Detection","sentence":"This is in contrast with the 5D case, where the spin-dependent $B^(1)_μ$-nucleus elastic scattering cross section is typically three or four orders of magnitude larger than the corresponding spin-independent cross section [ref] , and only the average over the nucleons inside the nucleus suppresses the spin-dependent effects.","intent_p":0.97,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":63,"sentences":66,"quotes":[{"arxiv_id":"1109.2587","title":"Collisions of Jets of Particles from Active Galactic Nuclei with Neutralino Dark Matter","url":"/paper/1109.2587","section":"Introduction","sentence":"Such a situation is common in the most popular theories of dark matter, such as in supersymmetric theories in which a neutralino plays the role of dark matter [ref] , and which can be up-scattered by an energetic beam electron into a selectron [Similarly, in theories with Universal Extra Dimensions [ref] , the dark matter particle may be a Kaluza-Klein excitation of the hypercharge vector boson [ref] , which may up-scatter into a Kaluza-Klein mode of the electron [ref] .] and was first proposed by [ref] and recently studied in [ref] .","intent_p":0.84,"contests_p":null},{"arxiv_id":"1910.02322","title":"Addressing $\\gamma$-ray emissions from dark matter annihilations in 45 milky way satellite galaxies and in extragalactic sources with particle dark matter models","url":"/paper/1910.02322","section":"Introduction","sentence":"In this work, we consider a KK dark matter candidate in an extra dimensional model namely Universal Extra Dimensional model (UED) [ref] .","intent_p":0.91,"contests_p":null},{"arxiv_id":"1007.0025","title":"5D UED: Flat and Flavorless","url":"/paper/1007.0025","section":"Introduction","sentence":"Another important development was the realization that there could be a geometric origin for the stability of a weakly interacting massive particle (WIMP) dark matter via Kaluza-Klein (KK) parity [ref] .","intent_p":0.89,"contests_p":null},{"arxiv_id":"1101.5205","title":"Introduction to dark matter experiments","url":"/paper/1101.5205","section":"Introduction","sentence":"Whatever physics solves the hierarchy problem associated with this symmetry breaking – be it supersymmetry [ref] , extra dimensions [ref] , or something else – gives rise to additional particles.","intent_p":0.86,"contests_p":null},{"arxiv_id":"0908.0899","title":"Kaluza-Klein Dark Matter And Neutrinos From Annihilation In The Sun","url":"/paper/0908.0899","section":"Introduction","sentence":"The phenomenology of a $B^(1)$ LKP has been studied extensively [ref] , including the prospects for direct [ref] and indirect detection [ref] .","intent_p":0.92,"contests_p":null}]}],"unlabelled_sentences":78},"outgoing":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"claims":[],"thresholds":{"intent_p":0.8,"supports_p":0.95,"contests_p":0.7},"method":"Citing sentences come from each paper's LaTeX source; every \\cite marks the sentence and the works it cites. Pith's classifier typed each sentence. A label is shown at intent probability 0.8 or more (0.95 for support), a contest at 0.7 or more. Measured accuracy against two blind model families is at https://pith.science/accuracy. The quoted sentences are the citing authors' own.","held_up":{"arxiv_id":"hep-ph/0207125","kind":"model","paper_version":2,"prompt_version":"held-up-v3.5","generated_at":"2026-10-27T15:46:32+00:00","loaded_at":"2026-10-28T01:02:29.085493+00:00","evidence":"some","account":[],"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":2,"entries":[{"p":0.92,"quote":null,"citing":[{"self":false,"year":2019,"title":"Addressing $\\gamma$-ray emissions from dark matter annihilations in 45 milky way satellite galaxies and in extragalactic sources with particle dark matter models","arxiv_id":"1910.02322"}],"verified":true,"paraphrase":"Computed the B1 B1 to qq annihilation cross-section from this paper's expression."},{"p":1.0,"quote":null,"citing":[{"self":false,"year":2007,"title":"WIMP identification through a combined measurement of axial and scalar couplings","arxiv_id":"0705.2502"}],"verified":true,"paraphrase":"Closely followed this paper in its calculation of the LKP scattering cross section off nucleons."}],"papers_all":4,"self_papers":0,"self_entries":[]}],"counts":{"by_kind":{"comparison":6,"method_or_tool":4,"supports_this_paper":1},"dropped":{"relied_on":0,"unknown_ids":0,"account_lines":0,"contest_vetoed":0,"below_threshold":0,"contest_drawback":0,"contest_without_basis":0,"contest_not_one_sentence":0,"contest_on_group_citation":0},"papers_read":7,"self_papers":17,"citing_papers":134,"sentences_read":9,"citing_sentences":168,"unambiguous_read":9,"typed_independent":7,"independent_papers":117,"by_kind_independent":{"comparison":4,"method_or_tool":3}},"input_sha256":"7f9cd9e4c1cf736fc0bf9c7eae0da6947e4558b5221e34f7dce235a1b4d06afd","method":"For a paper with five or more citing arXiv papers, Pith selected up to 40 citing sentences its citation classifier typed, read those whose citation markers point at this paper alone, and wrote one paraphrase for each later paper in each group, each resting on one sentence. A later paper is listed under a label only when the classifier gives one of its sentences that label at intent probability 0.8 or more (0.95 for support), Pith's reading of the sentence finds that the citing paper itself did it, and a second check of the paraphrase against the sentence passes. The section lists uses only: building on the paper, using its method, tool, data or values, comparing with it and citing it as support. It does not list criticism or disagreement, so their absence says nothing about how the paper has been received. Code counted the papers, wrote the summary from the listed entries, set the evidence level and linked each entry to its citing paper. Quotes are copied from the citing sentence and shown only when the citing paper's licence is CC BY, CC BY-SA or CC0; otherwise the paraphrase is shown. Papers that share an author with this one are listed apart. A paper with fewer citing papers gets a line counted by code, which names uses only: a later paper whose only label is a contest is counted as not described.","line":null,"summary":"2 later papers by other authors are listed below: 2 used its method or tool."},"_links":{"html":"https://pith.science/paper/hep-ph/0207125"}}