Home > Publications database > Search for Ultraheavy Dark Matter from Observations of Dwarf Spheroidal Galaxies with VERITAS > print |
001 | 576705 | ||
005 | 20230319000437.0 | ||
024 | 7 | _ | |a VERITAS:2023laq |2 INSPIRETeX |
024 | 7 | _ | |a inspire:2634024 |2 inspire |
024 | 7 | _ | |a arXiv:2302.08784 |2 arXiv |
024 | 7 | _ | |a altmetric:142723543 |2 altmetric |
037 | _ | _ | |a PUBDB-2023-00876 |
041 | _ | _ | |a English |
088 | _ | _ | |a arXiv:2302.08784 |2 arXiv |
100 | 1 | _ | |a Tak, Donggeun |0 P:(DE-H253)PIP1094637 |b 0 |e Corresponding author |
245 | _ | _ | |a Search for Ultraheavy Dark Matter from Observations of Dwarf Spheroidal Galaxies with VERITAS |
260 | _ | _ | |c 2023 |
336 | 7 | _ | |a Preprint |b preprint |m preprint |0 PUB:(DE-HGF)25 |s 1677572654_14761 |2 PUB:(DE-HGF) |
336 | 7 | _ | |a WORKING_PAPER |2 ORCID |
336 | 7 | _ | |a Electronic Article |0 28 |2 EndNote |
336 | 7 | _ | |a preprint |2 DRIVER |
336 | 7 | _ | |a ARTICLE |2 BibTeX |
336 | 7 | _ | |a Output Types/Working Paper |2 DataCite |
500 | _ | _ | |a 10 pages, 7 figures |
520 | _ | _ | |a Dark matter is a key piece of the current cosmological scenario, with weakly interacting massive particles (WIMPs) a leading dark matter candidate. WIMPs have not been detected in their conventional parameter space (100 GeV $\lesssim M_{\chi} \lesssim$ 100 TeV), a mass range accessible with current Imaging Atmospheric Cherenkov Telescopes. As ultraheavy dark matter (UHDM; $M_{\chi} \gtrsim$ 100 TeV) has been suggested as an under-explored alternative to the WIMP paradigm, we search for an indirect dark matter annihilation signal in a higher mass range (up to 30 PeV) with the VERITAS gamma-ray observatory. With 216 hours of observations of four dwarf spheroidal galaxies, we perform an unbinned likelihood analysis. We find no evidence of a $\gamma$-ray signal from UHDM annihilation above the background fluctuation for any individual dwarf galaxy nor for a joint-fit analysis, and consequently constrain the velocity-weighted annihilation cross section of UHDM for dark matter particle masses between 1 TeV and 30 PeV. We additionally set constraints on the allowed radius of a composite UHDM particle. |
536 | _ | _ | |a 613 - Matter and Radiation from the Universe (POF4-613) |0 G:(DE-HGF)POF4-613 |c POF4-613 |f POF IV |x 0 |
588 | _ | _ | |a Dataset connected to INSPIRE |
650 | _ | 7 | |a dark matter, annihilation |2 INSPIRE |
650 | _ | 7 | |a background, fluctuation |2 INSPIRE |
650 | _ | 7 | |a cross section, annihilation |2 INSPIRE |
650 | _ | 7 | |a WIMP |2 INSPIRE |
650 | _ | 7 | |a galaxy |2 INSPIRE |
650 | _ | 7 | |a TeV |2 INSPIRE |
650 | _ | 7 | |a VERITAS |2 INSPIRE |
650 | _ | 7 | |a observatory |2 INSPIRE |
650 | _ | 7 | |a GeV |2 INSPIRE |
650 | _ | 7 | |a composite |2 INSPIRE |
650 | _ | 7 | |a Cherenkov counter |2 INSPIRE |
650 | _ | 7 | |a imaging |2 INSPIRE |
650 | _ | 7 | |a gamma ray |2 INSPIRE |
693 | _ | _ | |0 EXP:(DE-H253)VERITAS-20170101 |5 EXP:(DE-H253)VERITAS-20170101 |e Very Energetic Radiation Imaging Telescope Array System |x 0 |
700 | 1 | _ | |a Pueschel, E. |0 P:(DE-H253)PIP1031007 |b 1 |e Corresponding author |u desy |
700 | 1 | _ | |a Baumgart, M. |0 M.Baumgart.1 |b 2 |
700 | 1 | _ | |a Rodd, N. L. |0 N.L.Rodd.1 |b 3 |
700 | 1 | _ | |a Acharyya, A. |b 4 |
700 | 1 | _ | |a Archer, A. |0 A.Archer.1 |b 5 |
700 | 1 | _ | |a Bangale, P. |0 P.Bangale.1 |b 6 |
700 | 1 | _ | |a Bartkoske, J. T. |0 J.T.Bartkoske.2 |b 7 |
700 | 1 | _ | |a Batista, P. |0 P.Batista.1 |b 8 |
700 | 1 | _ | |a Benbow, W. |0 W.Benbow.1 |b 9 |
700 | 1 | _ | |a Buckley, J. H. |0 James.H.Buckley.1 |b 10 |
700 | 1 | _ | |a Falcone, A. |0 A.Falcone.1 |b 11 |
700 | 1 | _ | |a Feng, Q. |b 12 |
700 | 1 | _ | |a Finley, J. P. |0 J.P.Finley.1 |b 13 |
700 | 1 | _ | |a Foote, G. M. |0 G.M.Foote.1 |b 14 |
700 | 1 | _ | |a Fortson, L. |0 L.F.Fortson.1 |b 15 |
700 | 1 | _ | |a Furniss, A. |0 A.K.Furniss.1 |b 16 |
700 | 1 | _ | |a Gallagher, G. |0 G.GallagherDaggitt.1 |b 17 |
700 | 1 | _ | |a Hanlon, W. F. |0 W.F.Hanlon.1 |b 18 |
700 | 1 | _ | |a Hervet, O. |0 O.Hervet.16 |b 19 |
700 | 1 | _ | |a Hoang, J. |0 J.Hoang.2 |b 20 |
700 | 1 | _ | |a Holder, J. |0 J.Holder.1 |b 21 |
700 | 1 | _ | |a Humensky, T. B. |0 T.B.Humensky.1 |b 22 |
700 | 1 | _ | |a Jin, W. |b 23 |
700 | 1 | _ | |a Kaaret, P. |0 P.Kaaret.1 |b 24 |
700 | 1 | _ | |a Kertzman, M. |0 M.Kertzman.6 |b 25 |
700 | 1 | _ | |a Kherlakian, M. |0 P:(DE-H253)PIP1084929 |b 26 |u desy |
700 | 1 | _ | |a Kieda, D. |0 D.B.Kieda.1 |b 27 |
700 | 1 | _ | |a Kleiner, T. K. |0 P:(DE-H253)PIP1093214 |b 28 |u desy |
700 | 1 | _ | |a Korzoun, N. |b 29 |
700 | 1 | _ | |a Krennrich, F. |0 F.Krennrich.1 |b 30 |
700 | 1 | _ | |a Lang, M. J. |b 31 |
700 | 1 | _ | |a Lundy, M. |0 M.Lundy.1 |b 32 |
700 | 1 | _ | |a Maier, G. |0 P:(DE-H253)PIP1011664 |b 33 |
700 | 1 | _ | |a McGrath, C. E. |0 C.E.McGrath.1 |b 34 |
700 | 1 | _ | |a Moriarty, P. |0 P.Moriarty.5 |b 35 |
700 | 1 | _ | |a O'Brien, S. |0 S.OBrien.4 |b 36 |
700 | 1 | _ | |a Ong, R. A. |b 37 |
700 | 1 | _ | |a Pfrang, K. |0 P:(DE-H253)PIP1083020 |b 38 |u desy |
700 | 1 | _ | |a Pohl, Martin |0 P:(DE-H253)PIP1010085 |b 39 |u desy |
700 | 1 | _ | |a Quinn, J. |0 John.Quinn.1 |b 40 |
700 | 1 | _ | |a Ragan, K. |0 K.J.Ragan.1 |b 41 |
700 | 1 | _ | |a Reynolds, P. T. |0 P.T.Reynolds.1 |b 42 |
700 | 1 | _ | |a Roache, E. |0 E.Roache.11 |b 43 |
700 | 1 | _ | |a Ryan, J. L. |0 J.L.Ryan.1 |b 44 |
700 | 1 | _ | |a Sadeh, I. |0 P:(DE-H253)PIP1006066 |b 45 |
700 | 1 | _ | |a Saha, L. |0 Lab.Saha.1 |b 46 |
700 | 1 | _ | |a Santander, M. |0 M.Santander.19 |b 47 |
700 | 1 | _ | |a Sembroski, G. H. |0 G.H.Sembroski.3 |b 48 |
700 | 1 | _ | |a Shang, R. |b 49 |
700 | 1 | _ | |a Splettstoesser, M. |0 Megan.Splettstoesser.1 |b 50 |
700 | 1 | _ | |a Tucci, J. V. |0 J.V.Tucci.1 |b 51 |
700 | 1 | _ | |a Vassiliev, V. V. |0 V.V.Vassiliev.2 |b 52 |
700 | 1 | _ | |a Williams, D. A. |0 D.A.Williams.1 |b 53 |
700 | 1 | _ | |a VERITAS Collaboration |0 P:(DE-HGF)0 |b 54 |e Collaboration Author |
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909 | C | O | |o oai:bib-pubdb1.desy.de:576705 |p VDB |
910 | 1 | _ | |a Deutsches Elektronen-Synchrotron |0 I:(DE-588b)2008985-5 |k DESY |b 0 |6 P:(DE-H253)PIP1094637 |
910 | 1 | _ | |a Deutsches Elektronen-Synchrotron |0 I:(DE-588b)2008985-5 |k DESY |b 1 |6 P:(DE-H253)PIP1031007 |
910 | 1 | _ | |a Deutsches Elektronen-Synchrotron |0 I:(DE-588b)2008985-5 |k DESY |b 26 |6 P:(DE-H253)PIP1084929 |
910 | 1 | _ | |a Deutsches Elektronen-Synchrotron |0 I:(DE-588b)2008985-5 |k DESY |b 28 |6 P:(DE-H253)PIP1093214 |
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913 | 1 | _ | |a DE-HGF |b Forschungsbereich Materie |l Matter and the Universe |1 G:(DE-HGF)POF4-610 |0 G:(DE-HGF)POF4-613 |3 G:(DE-HGF)POF4 |2 G:(DE-HGF)POF4-600 |4 G:(DE-HGF)POF |v Matter and Radiation from the Universe |x 0 |
914 | 1 | _ | |y 2023 |
915 | _ | _ | |a Published |0 StatID:(DE-HGF)0580 |2 StatID |
920 | 1 | _ | |0 I:(DE-H253)Z_VER-20210408 |k Z_VER |l VERITAS |x 0 |
980 | _ | _ | |a preprint |
980 | _ | _ | |a VDB |
980 | _ | _ | |a I:(DE-H253)Z_VER-20210408 |
980 | _ | _ | |a UNRESTRICTED |
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