Search for slow magnetic monopoles with the NOvA detector on the surface

We report a search for a magnetic monopole component of the cosmic-ray flux in a 95-day exposure of the NOvA experiment’s Far Detector, a 14 kt segmented liquid scintillator detector designed primarily to observe GeV-scale electron neutrinos. No events consistent with monopoles were observed, settin...

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Autores:
Acero, M. A.
Tipo de recurso:
Fecha de publicación:
2020
Institución:
Universidad del Atlántico
Repositorio:
Repositorio Uniatlantico
Idioma:
eng
OAI Identifier:
oai:repositorio.uniatlantico.edu.co:20.500.12834/798
Acceso en línea:
https://hdl.handle.net/20.500.12834/798
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openAccess
License
http://creativecommons.org/licenses/by-nc/4.0/
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oai_identifier_str oai:repositorio.uniatlantico.edu.co:20.500.12834/798
network_acronym_str UNIATLANT2
network_name_str Repositorio Uniatlantico
repository_id_str
dc.title.spa.fl_str_mv Search for slow magnetic monopoles with the NOvA detector on the surface
title Search for slow magnetic monopoles with the NOvA detector on the surface
spellingShingle Search for slow magnetic monopoles with the NOvA detector on the surface
title_short Search for slow magnetic monopoles with the NOvA detector on the surface
title_full Search for slow magnetic monopoles with the NOvA detector on the surface
title_fullStr Search for slow magnetic monopoles with the NOvA detector on the surface
title_full_unstemmed Search for slow magnetic monopoles with the NOvA detector on the surface
title_sort Search for slow magnetic monopoles with the NOvA detector on the surface
dc.creator.fl_str_mv Acero, M. A.
dc.contributor.author.none.fl_str_mv Acero, M. A.
dc.contributor.other.none.fl_str_mv Adamson, P.
Aliaga, L.
Alion, T.
Allakhverdian, V.
Anfimov, N.
Antoshkin, A.
Arrieta-Diaz, E.
Asquith, L.
Aurisano, A.
Back, A.
Backhouse, C.
Baird, M.
Balashov, N.
Baldi, P.
Bambah, B. A.
Bashar, S.
Bays, K.
Bending, S.
Bernstein, R.
Bhatnagar, V.
Bhuyan, B.
Bian, J.
Blair, J.
Booth, A. C.
Bour, P.
Bowle, R.
Bromberg, C.
Buchanan, N.
Butkevich, A.
Calvez, S.
Carroll, T. J.
Catano-Mur, E.
Childress, S.
Choudhary, B. C.
Coan, T. E.
Colo, M.
Corwin, L.
Cremonesi, L.
Davies, G. S.
Derwent, P. F.
Ding, P.
Djurcic, Z.
Dolce, M.
Doyle, D.
Dueñas Tonguino, D.
Dung, P.
Dukes, E. C.
Duyang, H.
Edayath, S.
Ehrlich, R.
Elkins, M.
Feldman, G. J.
Filip, P.
Flanagan, W.
Franc, J.
Frank, M. J.
Gallagher, H. R.
Gandrajula, R.
Gao, F.
Germani, S.
Giri, A.
Gomes, R. A.
Goodman, M. C.
Grichine, V.
Groh, M.
Group, R.
Guo, B.
Habig, A.
Hakl, F.
Hall, A.
Hartnell, J.
Hatcher, R.
Heller, K.
Hewes, J.
Himmel, A.
Holin, A.
Huang, J.
Hylen, J.
Jarosz, J.
Jediny, F.
Johnson, C.
Judah, M.
Kakorin, I.
Kalra, D.
Kaplan, D. M.
Keloth, R.
Klimov, O.
Koerner, L. W.
Kolupaeva, L.
Kotelnikov, S.
Kullenberg, Ch.
Kubu, M.
Kumar, A.
Kuruppu, C. D.
Kus, V.
Lackey, T.
Lang, K.
Li, L.
Lin, S.
Lister, A.
Lokajicek, M.
Luchuk, S.
Magill, S.
Mann, W. A.
Marshak, M. L.
Martinez-Casales, M.
Matveev, V.
Mayes, B.
Méndez, D. P.
Messier, M. D.
Meyer, H.
Miao, T.
Miller, W. H.
Mishra, S. R.
Mislivec, A.
Mohanta, R.
Moren, A.
Morozova, A.
Mualem, L.
Muether, M.
Mufson, S.
Mulder, K.
Murphy, R.
Musser, J.
Naples, D.
Nayak, N.
Nelson, J. K.
Nichol, R.
Niner, E.
Norman, A.
Norrick, A.
Nosek, T.
Olshevskiy, A.
Olson, T.
Paley, J.
Patterson, R. B.
Pawloski, G.
Petrova, O.
Petti, R.
Plunkett, R. K.
Rafique, A.
Raj, V.
Ramson, B.
Rebel, B.
Rojas, P.
Ryabov, V.
Samoylov, O.
Sanchez, M. C.
Sánchez Falero, S.
Shanahan, P.
Sheshukov, A.
Singh, P.
Singh, V.
Smith, E.
Smolik, J.
Snopok, P.
Solomey, N.
Song, E.
Sousa, A.
Soustruznik, K.
Strait, M.
Suter, L.
Sutton, A.
Swain, S.
Sweeney, C.
Tapia Oregui, B.
Tas, P.
Thayyullathi, R. B.
Thomas, J.
Tiras, E.
Torbunov, D.
Tripathi, J.
Trokan-Tenorio, J.
Torun, Y.
Urheim, J.
Vahle, P.
Vallar, Z.
Vasel, J.
Vokac, P.
Vrba, T.
Wallbank, M.
Wang, Z.
Warburton, T. K.
Wetstein, M.
Whittington, D.
Wickremasinghe, D. A.
Wojcicki, S. G.
Wolcott, J.
Xiao, Y.
Yallappa Dombara, A.
Yonehara, K.
Yu, S.
Yu, Y.
Zadorozhnyy, S.
Zalesak, J.
Zhang, Y.
Zwaska, R.
description We report a search for a magnetic monopole component of the cosmic-ray flux in a 95-day exposure of the NOvA experiment’s Far Detector, a 14 kt segmented liquid scintillator detector designed primarily to observe GeV-scale electron neutrinos. No events consistent with monopoles were observed, setting an upper limit on the flux of 2 ×10−14 cm−2 s −1 sr−1 at 90% C.L. for monopole speed 6 × 10−4 < β < 5 × 10−3 and mass greater than 5 × 108 GeV. Because of NOvA’s small overburden of 3 meters-water equivalent, this constraint covers a previously unexplored low-mass region.
publishDate 2020
dc.date.submitted.none.fl_str_mv 2020-12-15
dc.date.issued.none.fl_str_mv 2021-01-05
dc.date.accessioned.none.fl_str_mv 2022-11-15T19:21:23Z
dc.date.available.none.fl_str_mv 2022-11-15T19:21:23Z
dc.type.coarversion.fl_str_mv http://purl.org/coar/version/c_970fb48d4fbd8a85
dc.type.coar.fl_str_mv http://purl.org/coar/resource_type/c_2df8fbb1
dc.type.driver.spa.fl_str_mv info:eu-repo/semantics/article
dc.type.hasVersion.spa.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.spa.spa.fl_str_mv Artículo
status_str publishedVersion
dc.identifier.uri.none.fl_str_mv https://hdl.handle.net/20.500.12834/798
dc.identifier.doi.none.fl_str_mv 10.1103/PhysRevD.103.012007
dc.identifier.instname.spa.fl_str_mv Universidad del Atlántico
dc.identifier.reponame.spa.fl_str_mv Repositorio Universidad del Atlántico
url https://hdl.handle.net/20.500.12834/798
identifier_str_mv 10.1103/PhysRevD.103.012007
Universidad del Atlántico
Repositorio Universidad del Atlántico
dc.language.iso.spa.fl_str_mv eng
language eng
dc.rights.coar.fl_str_mv http://purl.org/coar/access_right/c_abf2
dc.rights.uri.*.fl_str_mv http://creativecommons.org/licenses/by-nc/4.0/
dc.rights.cc.*.fl_str_mv Attribution-NonCommercial 4.0 International
dc.rights.accessRights.spa.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc/4.0/
Attribution-NonCommercial 4.0 International
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eu_rights_str_mv openAccess
dc.format.mimetype.spa.fl_str_mv application/pdf
dc.publisher.place.spa.fl_str_mv Barranquilla
dc.publisher.sede.spa.fl_str_mv Sede Norte
institution Universidad del Atlántico
bitstream.url.fl_str_mv https://repositorio.uniatlantico.edu.co/bitstream/20.500.12834/798/1/PhysRevD.103.012007.pdf
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spelling Acero, M. A.979f9c6a-faae-415d-b017-8ea1e9afa74cAdamson, P.Aliaga, L.Alion, T.Allakhverdian, V.Anfimov, N.Antoshkin, A.Arrieta-Diaz, E.Asquith, L.Aurisano, A.Back, A.Backhouse, C.Baird, M.Balashov, N.Baldi, P.Bambah, B. A.Bashar, S.Bays, K.Bending, S.Bernstein, R.Bhatnagar, V.Bhuyan, B.Bian, J.Blair, J.Booth, A. C.Bour, P.Bowle, R.Bromberg, C.Buchanan, N.Butkevich, A.Calvez, S.Carroll, T. J.Catano-Mur, E.Childress, S.Choudhary, B. C.Coan, T. E.Colo, M.Corwin, L.Cremonesi, L.Davies, G. S.Derwent, P. F.Ding, P.Djurcic, Z.Dolce, M.Doyle, D.Dueñas Tonguino, D.Dung, P.Dukes, E. C.Duyang, H.Edayath, S.Ehrlich, R.Elkins, M.Feldman, G. J.Filip, P.Flanagan, W.Franc, J.Frank, M. J.Gallagher, H. R.Gandrajula, R.Gao, F.Germani, S.Giri, A.Gomes, R. A.Goodman, M. C.Grichine, V.Groh, M.Group, R.Guo, B.Habig, A.Hakl, F.Hall, A.Hartnell, J.Hatcher, R.Heller, K.Hewes, J.Himmel, A.Holin, A.Huang, J.Hylen, J.Jarosz, J.Jediny, F.Johnson, C.Judah, M.Kakorin, I.Kalra, D.Kaplan, D. M.Keloth, R.Klimov, O.Koerner, L. W.Kolupaeva, L.Kotelnikov, S.Kullenberg, Ch.Kubu, M.Kumar, A.Kuruppu, C. D.Kus, V.Lackey, T.Lang, K.Li, L.Lin, S.Lister, A.Lokajicek, M.Luchuk, S.Magill, S.Mann, W. A.Marshak, M. L.Martinez-Casales, M.Matveev, V.Mayes, B.Méndez, D. P.Messier, M. D.Meyer, H.Miao, T.Miller, W. H.Mishra, S. R.Mislivec, A.Mohanta, R.Moren, A.Morozova, A.Mualem, L.Muether, M.Mufson, S.Mulder, K.Murphy, R.Musser, J.Naples, D.Nayak, N.Nelson, J. K.Nichol, R.Niner, E.Norman, A.Norrick, A.Nosek, T.Olshevskiy, A.Olson, T.Paley, J.Patterson, R. B.Pawloski, G.Petrova, O.Petti, R.Plunkett, R. K.Rafique, A.Raj, V.Ramson, B.Rebel, B.Rojas, P.Ryabov, V.Samoylov, O.Sanchez, M. C.Sánchez Falero, S.Shanahan, P.Sheshukov, A.Singh, P.Singh, V.Smith, E.Smolik, J.Snopok, P.Solomey, N.Song, E.Sousa, A.Soustruznik, K.Strait, M.Suter, L.Sutton, A.Swain, S.Sweeney, C.Tapia Oregui, B.Tas, P.Thayyullathi, R. B.Thomas, J.Tiras, E.Torbunov, D.Tripathi, J.Trokan-Tenorio, J.Torun, Y.Urheim, J.Vahle, P.Vallar, Z.Vasel, J.Vokac, P.Vrba, T.Wallbank, M.Wang, Z.Warburton, T. K.Wetstein, M.Whittington, D.Wickremasinghe, D. A.Wojcicki, S. G.Wolcott, J.Xiao, Y.Yallappa Dombara, A.Yonehara, K.Yu, S.Yu, Y.Zadorozhnyy, S.Zalesak, J.Zhang, Y.Zwaska, R.2022-11-15T19:21:23Z2022-11-15T19:21:23Z2021-01-052020-12-15https://hdl.handle.net/20.500.12834/79810.1103/PhysRevD.103.012007Universidad del AtlánticoRepositorio Universidad del AtlánticoWe report a search for a magnetic monopole component of the cosmic-ray flux in a 95-day exposure of the NOvA experiment’s Far Detector, a 14 kt segmented liquid scintillator detector designed primarily to observe GeV-scale electron neutrinos. No events consistent with monopoles were observed, setting an upper limit on the flux of 2 ×10−14 cm−2 s −1 sr−1 at 90% C.L. for monopole speed 6 × 10−4 < β < 5 × 10−3 and mass greater than 5 × 108 GeV. Because of NOvA’s small overburden of 3 meters-water equivalent, this constraint covers a previously unexplored low-mass region.application/pdfenghttp://creativecommons.org/licenses/by-nc/4.0/Attribution-NonCommercial 4.0 Internationalinfo:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_abf2Search for slow magnetic monopoles with the NOvA detector on the surfacePúblico generalinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArtículohttp://purl.org/coar/version/c_970fb48d4fbd8a85http://purl.org/coar/resource_type/c_2df8fbb1BarranquillaSede Norte[1] P. A. M. Dirac, Proc. Roy. Soc. Lond. A133, 60 (1931).[2] M. Tanabashi et al. (Particle Data Group), Phys. Rev. D98, 030001 (2018).[3] G. ’t Hooft, Nucl. Phys. B 79, 276 (1974)[4] A. M. Polyakov, JETP Lett. 20, 194 (1974).[5] T. W. Kephart and Q. Shafi, Phys. Lett. B520, 313 (2001), arXiv:hep-ph/0105237 [hep-ph].[6] D. E. Groom, In search of the supermassive magnetic monopole, Phys. Rep. 140, 323 (1986)[7] M. Ambrosio et al. (MACRO Collaboration), Final results of magnetic monopole searches with the MACRO experiment, Eur. Phys. J. C 25, 511 (2002).[8] S. Balestra et al., Magnetic monopole search at high altitude with the SLIM experiment, Eur. Phys. J. C 55, 57 (2008)[9] M. Acero et al. (NOvA Collaboration), First Measurement of Neutrino Oscillation Parameters Using Neutrinos and Antineutrinos by NOvA, Phys. Rev. Lett. 123, 151803 (2019).[10] D. S. Ayres et al. (NOvA Collaboration), The NOvA technical design report, Report No. FERMI-LAB-DESIGN-2007-01, 2007, https://doi.org/10.2172/935497.[11] V. A. Rubakov, Superheavy magnetic monopoles and proton decay, Pis’ma Zh. Eksp. Teor. Fiz. 33, 658 (1981) [JETP Lett. 33, 644 (1981)][12] S. P. Ahlen and K. Kinoshita, Calculation of the stopping power of very-low-velocity magnetic monopoles, Phys. Rev. D 26, 2347 (1982).[13] S. Mufson et al., Liquid scintillator production for the NOvA experiment, Nucl. Instrum. Methods Phys. Res., Sect. A 799, 1 (2015)[13] S. Mufson et al., Liquid scintillator production for the NOvA experiment, Nucl. Instrum. Methods Phys. Res., Sect. A 799, 1 (2015)[15] A. Aurisano, C. Backhouse, R. Hatcher, N. Mayer, J. Musser, R. Patterson, R. Schroeter, and A. Sousa (NOvA Collaboration), The NOvA simulation chain, J. Phys. Conf. Ser. 664, 072002 (2015).[16] A. Norman et al., Performance of the NOvA data acquisition and trigger systems for the full 14 kt far detector, J. Phys. Conf. Ser. 664, 082041 (2015).[17] P. Hough, Method and means for recognizing complex patterns, U.S. Patent No. 3069654 (1962).[18] R. Abbasi et al. (IceCube Collaboration), Search for relativistic magnetic monopoles with IceCube, Phys. Rev. D 87, 022001 (2013).[19] M. G. Aartsen et al. (IceCube Collaboration), Search for non-relativistic magnetic monopoles with IceCube, Eur. Phys. J. C 74, 2938 (2014); 79, 124(E) (2019).[20] D. P. Hogan, D. Z. Besson, J. P. Ralston, I. Kravchenko, and D. Seckel, Relativistic magnetic monopole flux constraints from RICE, Phys. Rev. D 78, 075031 (2008)[21] Z. Wang, Search for magnetic monopoles with the NOvA far detector, Ph.D. thesis, University of Virginia, 2015, https://doi.org/10.2172/1230047http://purl.org/coar/resource_type/c_6501ORIGINALPhysRevD.103.012007.pdfPhysRevD.103.012007.pdfapplication/pdf736756https://repositorio.uniatlantico.edu.co/bitstream/20.500.12834/798/1/PhysRevD.103.012007.pdfb935938343a9d205c70d3234d0171a1fMD51CC-LICENSElicense_rdflicense_rdfapplication/rdf+xml; charset=utf-8914https://repositorio.uniatlantico.edu.co/bitstream/20.500.12834/798/2/license_rdf24013099e9e6abb1575dc6ce0855efd5MD52LICENSElicense.txtlicense.txttext/plain; charset=utf-81306https://repositorio.uniatlantico.edu.co/bitstream/20.500.12834/798/3/license.txt67e239713705720ef0b79c50b2ececcaMD5320.500.12834/798oai:repositorio.uniatlantico.edu.co:20.500.12834/7982022-11-15 14:21:24.123DSpace de la Universidad de Atlánticosysadmin@mail.uniatlantico.edu.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