Matches in SemOpenAlex for { <https://semopenalex.org/work/W3217672740> ?p ?o ?g. }
- W3217672740 abstract "We explore the possibility that relativistic protons in the extremely powerful jets of blazars may boost via elastic collisions the dark matter particles in the surroundings of the source to high energies. We concentrate on two sample blazars, TXS 0506+056, towards which IceCube recently reported evidence for a high-energy neutrino flux, and BL Lacertae, a representative nearby blazar. We find that the dark matter flux at Earth induced by these sources may be sizable, larger than the flux associated with the analogous process of dark matter boosted by galactic cosmic rays, and relevant to access direct detection for dark matter particle masses lighter than 1 GeV. From the null detection of a signal by XENON1T, MiniBooNE, and Borexino, we derive limits on dark matter-nucleus spin-independent and spin-dependent cross sections which, depending on the modelization of the source, improve on other currently available bounds for light dark matter candidates of 1 up to 5 orders of magnitude." @default.
- W3217672740 created "2021-12-06" @default.
- W3217672740 creator A5012107958 @default.
- W3217672740 creator A5043304911 @default.
- W3217672740 creator A5081130819 @default.
- W3217672740 date "2022-06-03" @default.
- W3217672740 modified "2023-09-30" @default.
- W3217672740 title "Direct Detection Constraints on Blazar-Boosted Dark Matter" @default.
- W3217672740 cites W1487701853 @default.
- W3217672740 cites W1669035376 @default.
- W3217672740 cites W1677429399 @default.
- W3217672740 cites W1951204806 @default.
- W3217672740 cites W1953516118 @default.
- W3217672740 cites W1979115990 @default.
- W3217672740 cites W2036385708 @default.
- W3217672740 cites W2043145737 @default.
- W3217672740 cites W2047159064 @default.
- W3217672740 cites W2051180132 @default.
- W3217672740 cites W2056313509 @default.
- W3217672740 cites W2067748843 @default.
- W3217672740 cites W2070577141 @default.
- W3217672740 cites W2088868638 @default.
- W3217672740 cites W2092243462 @default.
- W3217672740 cites W2092551259 @default.
- W3217672740 cites W2099693814 @default.
- W3217672740 cites W2102639000 @default.
- W3217672740 cites W2118125580 @default.
- W3217672740 cites W2124833255 @default.
- W3217672740 cites W2135101687 @default.
- W3217672740 cites W2139162812 @default.
- W3217672740 cites W2148569062 @default.
- W3217672740 cites W2149990597 @default.
- W3217672740 cites W2152242740 @default.
- W3217672740 cites W2169080969 @default.
- W3217672740 cites W2214680270 @default.
- W3217672740 cites W2548793783 @default.
- W3217672740 cites W2553636544 @default.
- W3217672740 cites W2731029008 @default.
- W3217672740 cites W2746829047 @default.
- W3217672740 cites W2747943382 @default.
- W3217672740 cites W2756902241 @default.
- W3217672740 cites W2758606062 @default.
- W3217672740 cites W2786110165 @default.
- W3217672740 cites W2786527709 @default.
- W3217672740 cites W2786980339 @default.
- W3217672740 cites W2787379565 @default.
- W3217672740 cites W2788362179 @default.
- W3217672740 cites W2795533374 @default.
- W3217672740 cites W2801053672 @default.
- W3217672740 cites W2809170714 @default.
- W3217672740 cites W2848424442 @default.
- W3217672740 cites W2848722098 @default.
- W3217672740 cites W2873976311 @default.
- W3217672740 cites W2898095785 @default.
- W3217672740 cites W2914120085 @default.
- W3217672740 cites W2929611936 @default.
- W3217672740 cites W3011243017 @default.
- W3217672740 cites W3093690346 @default.
- W3217672740 cites W3100256087 @default.
- W3217672740 cites W3102561241 @default.
- W3217672740 cites W3103507618 @default.
- W3217672740 cites W3104111652 @default.
- W3217672740 cites W3105280224 @default.
- W3217672740 cites W3114651388 @default.
- W3217672740 cites W3124047548 @default.
- W3217672740 cites W4210367512 @default.
- W3217672740 cites W4288079944 @default.
- W3217672740 doi "https://doi.org/10.1103/physrevlett.128.221104" @default.
- W3217672740 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/35714241" @default.
- W3217672740 hasPublicationYear "2022" @default.
- W3217672740 type Work @default.
- W3217672740 sameAs 3217672740 @default.
- W3217672740 citedByCount "15" @default.
- W3217672740 countsByYear W32176727402021 @default.
- W3217672740 countsByYear W32176727402022 @default.
- W3217672740 countsByYear W32176727402023 @default.
- W3217672740 crossrefType "journal-article" @default.
- W3217672740 hasAuthorship W3217672740A5012107958 @default.
- W3217672740 hasAuthorship W3217672740A5043304911 @default.
- W3217672740 hasAuthorship W3217672740A5081130819 @default.
- W3217672740 hasBestOaLocation W32176727402 @default.
- W3217672740 hasConcept C100752510 @default.
- W3217672740 hasConcept C103193775 @default.
- W3217672740 hasConcept C107966497 @default.
- W3217672740 hasConcept C109214941 @default.
- W3217672740 hasConcept C113840448 @default.
- W3217672740 hasConcept C121332964 @default.
- W3217672740 hasConcept C159249277 @default.
- W3217672740 hasConcept C172790937 @default.
- W3217672740 hasConcept C186453547 @default.
- W3217672740 hasConcept C191897082 @default.
- W3217672740 hasConcept C192562407 @default.
- W3217672740 hasConcept C26405456 @default.
- W3217672740 hasConcept C26495451 @default.
- W3217672740 hasConcept C2778810938 @default.
- W3217672740 hasConcept C44870925 @default.
- W3217672740 hasConcept C57853336 @default.
- W3217672740 hasConcept C66157390 @default.
- W3217672740 hasConcept C68709404 @default.
- W3217672740 hasConcept C78470386 @default.