{"arxiv_id":"hep-ph/0009083","incoming":{"papers":92,"sentences":121,"groups":[{"kind":"comparison","label":"Compares with it","papers":3,"sentences":3,"quotes":[{"arxiv_id":"2008.11686","title":"Einstein-Cartan Portal to Dark Matter","url":"/paper/2008.11686","section":"Introduction","sentence":"We see that the DM momentum distribution ([ref]) has a unique form and differs from both non-resonantly [ref] and resonantly produced sterile neutrinos [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"2411.07029","title":"Cosmological Constraints on Dark Neutrino Towers","url":"/paper/2411.07029","section":"Conclusions","sentence":"The additional suppression factor which we have bounded to be $ζ0.01$ is consistent with the estimates obtained in 4D sterile neutrino models; see e.g. [ref] .","intent_p":0.9,"contests_p":null},{"arxiv_id":"1609.07647","title":"Production of heavy sterile neutrinos from vector boson decay at electroweak temperatures","url":"/paper/1609.07647","section":"Comparison to other results","sentence":"The final form of the quantum kinetic equation ([ref]) is similar to that used in [ref] , although in these articles the mixing angle only includes the index of refraction (real part), valid in the temperature regime of interest in those articles.","intent_p":0.9,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites it as support","papers":2,"sentences":2,"quotes":[{"arxiv_id":"2107.02803","title":"Gauged Inverse Seesaw from Dark Matter","url":"/paper/2107.02803","section":"Scalar dark matter","sentence":"However, it is interesting to note that both the annihilation and the coannihilation into active neutrinos depends on the active-sterile mixing angles (to the fourth power), which are suppressed at high temperature (i.e. at $T ≳200$ MeV) due to over dominating thermal masses of the active neutrinos [ref] , and therefore these channels are subdominant.","intent_p":0.96,"contests_p":null},{"arxiv_id":"2007.08863","title":"Light Majorana Neutrinos in (Semi)invisible Meson Decays","url":"/paper/2007.08863","section":"Introduction","sentence":"Massive neutral fermions which are long lived enough compared to the age of the universe and have mass in the range $2keV ≲m_N_k ≲5keV$ [ref] are good warm dark matter candidates [ref] .","intent_p":0.96,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":37,"sentences":43,"quotes":[{"arxiv_id":"0803.2735","title":"MeV sterile neutrinos in low reheating temperature cosmological scenarios","url":"/paper/0803.2735","section":"Introduction","sentence":"Dodelson and Widrow [ref] (see also Refs. [ref] ) provided the first analytical calculation of the production of sterile neutrinos lighter than 100 keV in the early Universe, under the assumption (which we maintain here) of a negligible primordial lepton asymmetry.","intent_p":0.8,"contests_p":null},{"arxiv_id":"1006.4008","title":"Resonant production of the sterile neutrino dark matter and fine-tunings in the [nu]MSM","url":"/paper/1006.4008","section":"Introduction","sentence":"The spectrum and the number density of produced particles depends essentially on three parameters: the mixing angle with ordinary neutrino, the sterile neutrino mass and the lepton asymmetry of the Universe ($ΔL$) at the production time (for a recent analysis, see [ref] ; earlier considerations can be found in [ref] ).","intent_p":0.81,"contests_p":null},{"arxiv_id":"1111.4217","title":"Constraining Sterile Neutrino Warm Dark Matter with Chandra Observations of the Andromeda Galaxy","url":"/paper/1111.4217","section":"Introduction","sentence":"Sterile neutrinos may also play the role of the dark matter, e.g., [ref] and affect a host of interesting cosmological and astrophysical processes, including the production of baryon [ref] and lepton [ref] asymmetries, Big Bang Nucleosynthesis [ref] , the evolution of the matter power spectrum [ref] , reionization [ref] , neutrino oscillations [ref] , pulsar kicks [ref] , and supernovae [ref] .","intent_p":0.95,"contests_p":null},{"arxiv_id":"2309.13376","title":"Sterile Neutrino Dark Matter, Matter-Antimatter Separation, and the QCD Phase Transition","url":"/paper/2309.13376","section":"Introduction","sentence":"The proposals include the decays of extra scalar particles [ref] , higher-dimensional operators [ref] , Einstein-Cartan 4-fermion gravitational interaction [ref] , left-right symmetric theories [ref] etc.] In the case of small lepton asymmetries of the Universe (the Dodelson-Widrow mechanism [ref] ), the required mixing angle is in contradiction with X-ray[ $N_1$ is unstable and can decay as $N_1→γν$, producing a narrow X-ray line that can be seen by X-ray telescopes [ref] .","intent_p":0.96,"contests_p":null},{"arxiv_id":"1901.01262","title":"New Constraints on Sterile Neutrino Dark Matter from $NuSTAR$ M31 Observations","url":"/paper/1901.01262","section":"Introduction","sentence":"In the X-ray band, one of the most studied candidates is sterile neutrinos [ref] , which can radiatively decay into an active neutrino and a monoenergetic photon ($χ→γ+ ν$) with energy equal to half of the DM mass [ref] .","intent_p":0.96,"contests_p":null}]}],"unlabelled_sentences":73},"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/0009083","kind":"model","paper_version":3,"prompt_version":"held-up-v3.5","generated_at":"2026-10-27T16:44:55+00:00","loaded_at":"2026-10-28T01:02:47.851753+00:00","evidence":"some","account":[],"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":1,"entries":[{"p":0.82,"quote":null,"citing":[{"self":false,"year":2017,"title":"Sterile neutrino dark matter from right-handed neutrino oscillations","arxiv_id":"1702.04526"}],"verified":true,"paraphrase":"Used this paper's Boltzmann equation for ν_R1, with its collision term and oscillation probability, in its own treatment."}],"papers_all":1,"self_papers":0,"self_entries":[]}],"counts":{"by_kind":{"data_used":1,"comparison":3,"method_or_tool":1,"supports_this_paper":2},"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":1,"citing_papers":107,"sentences_read":7,"citing_sentences":147,"unambiguous_read":7,"typed_independent":7,"independent_papers":106,"by_kind_independent":{"data_used":1,"comparison":3,"method_or_tool":1,"supports_this_paper":2}},"input_sha256":"a711c7ee6084da3c74a351b2c2cd43546012e6cd69dd504aa71eb47dc8bbd6fd","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":"1 later paper by other authors is listed below: 1 used its method or tool."},"_links":{"html":"https://pith.science/paper/hep-ph/0009083"}}