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Search for Relativistic Magnetic Monopoles with Eight Years of IceCube Data.

Authors :
Abbasi R
Ackermann M
Adams J
Aguilar JA
Ahlers M
Ahrens M
Alispach C
Alves AA
Amin NM
An R
Andeen K
Anderson T
Anton G
Argüelles C
Ashida Y
Axani S
Bai X
Balagopal V A
Barbano A
Barwick SW
Bastian B
Basu V
Baur S
Bay R
Beatty JJ
Becker KH
Becker Tjus J
Bellenghi C
BenZvi S
Berley D
Bernardini E
Besson DZ
Binder G
Bindig D
Blaufuss E
Blot S
Boddenberg M
Bontempo F
Borowka J
Böser S
Botner O
Böttcher J
Bourbeau E
Bradascio F
Braun J
Bron S
Brostean-Kaiser J
Browne S
Burgman A
Burley RT
Busse RS
Campana MA
Carnie-Bronca EG
Chen C
Chen Z
Chirkin D
Choi K
Clark BA
Clark K
Classen L
Coleman A
Collin GH
Conrad JM
Coppin P
Correa P
Cowen DF
Cross R
Dappen C
Dave P
De Clercq C
DeLaunay JJ
Dembinski H
Deoskar K
Desai A
Desiati P
de Vries KD
de Wasseige G
de With M
DeYoung T
Dharani S
Diaz A
Díaz-Vélez JC
Dittmer M
Dujmovic H
Dunkman M
DuVernois MA
Dvorak E
Ehrhardt T
Eller P
Engel R
Erpenbeck H
Evans J
Evenson PA
Fan KL
Fazely AR
Feigl N
Fiedlschuster S
Fienberg AT
Filimonov K
Finley C
Fischer L
Fox D
Franckowiak A
Friedman E
Fritz A
Fürst P
Gaisser TK
Gallagher J
Ganster E
Garcia A
Garrappa S
Gerhardt L
Ghadimi A
Glaser C
Glauch T
Glüsenkamp T
Gonzalez JG
Goswami S
Grant D
Grégoire T
Griswold S
Gündüz M
Günther C
Haack C
Hallgren A
Halliday R
Halve L
Halzen F
Ha Minh M
Hanson K
Hardin J
Harnisch AA
Haungs A
Hauser S
Hebecker D
Helbing K
Henningsen F
Hettinger EC
Hickford S
Hignight J
Hill C
Hill GC
Hoffman KD
Hoffmann R
Hoinka T
Hokanson-Fasig B
Hoshina K
Huang F
Huber M
Huber T
Hultqvist K
Hünnefeld M
Hussain R
In S
Iovine N
Ishihara A
Jansson M
Japaridze GS
Jeong M
Jones BJP
Kang D
Kang W
Kang X
Kappes A
Kappesser D
Karg T
Karl M
Karle A
Katz U
Kauer M
Kellermann M
Kelley JL
Kheirandish A
Kin K
Kintscher T
Kiryluk J
Klein SR
Koirala R
Kolanoski H
Kontrimas T
Köpke L
Kopper C
Kopper S
Koskinen DJ
Koundal P
Kovacevich M
Kowalski M
Kozynets T
Kun E
Kurahashi N
Lad N
Lagunas Gualda C
Lanfranchi JL
Larson MJ
Lauber F
Lazar JP
Lee JW
Leonard K
Leszczyńska A
Li Y
Lincetto M
Liu QR
Liubarska M
Lohfink E
Lozano Mariscal CJ
Lu L
Lucarelli F
Ludwig A
Luszczak W
Lyu Y
Ma WY
Madsen J
Mahn KBM
Makino Y
Mancina S
Mariş IC
Maruyama R
Mase K
McElroy T
McNally F
Mead JV
Meagher K
Mechbal S
Medina A
Meier M
Meighen-Berger S
Micallef J
Mockler D
Montaruli T
Moore RW
Morse R
Moulai M
Naab R
Nagai R
Naumann U
Necker J
Nguyễn LV
Niederhausen H
Nisa MU
Nowicki SC
Obertacke Pollmann A
Oehler M
Oeyen B
Olivas A
O'Sullivan E
Pandya H
Pankova DV
Park N
Parker GK
Paudel EN
Paul L
Pérez de Los Heros C
Peters L
Peterson J
Philippen S
Pieloth D
Pieper S
Pittermann M
Pizzuto A
Plum M
Popovych Y
Porcelli A
Prado Rodriguez M
Price PB
Pries B
Przybylski GT
Raab C
Raissi A
Rameez M
Rawlins K
Rea IC
Rehman A
Reichherzer P
Reimann R
Renzi G
Resconi E
Reusch S
Rhode W
Richman M
Riedel B
Roberts EJ
Robertson S
Roellinghoff G
Rongen M
Rott C
Ruhe T
Ryckbosch D
Rysewyk Cantu D
Safa I
Saffer J
Sanchez Herrera SE
Sandrock A
Sandroos J
Santander M
Sarkar S
Sarkar S
Satalecka K
Scharf M
Schaufel M
Schieler H
Schindler S
Schlunder P
Schmidt T
Schneider A
Schneider J
Schröder FG
Schumacher L
Schwefer G
Sclafani S
Seckel D
Seunarine S
Sharma A
Shefali S
Silva M
Skrzypek B
Smithers B
Snihur R
Soedingrekso J
Soldin D
Spannfellner C
Spiczak GM
Spiering C
Stachurska J
Stamatikos M
Stanev T
Stein R
Stettner J
Steuer A
Stezelberger T
Stürwald T
Stuttard T
Sullivan GW
Taboada I
Tenholt F
Ter-Antonyan S
Tilav S
Tischbein F
Tollefson K
Tomankova L
Tönnis C
Toscano S
Tosi D
Trettin A
Tselengidou M
Tung CF
Turcati A
Turcotte R
Turley CF
Twagirayezu JP
Ty B
Unland Elorrieta MA
Valtonen-Mattila N
Vandenbroucke J
van Eijndhoven N
Vannerom D
van Santen J
Verpoest S
Walck C
Watson TB
Weaver C
Weigel P
Weindl A
Weiss MJ
Weldert J
Wendt C
Werthebach J
Weyrauch M
Whitehorn N
Wiebusch CH
Williams DR
Wolf M
Woschnagg K
Wrede G
Wulff J
Xu XW
Yanez JP
Yoshida S
Yu S
Yuan T
Zhang Z
Source :
Physical review letters [Phys Rev Lett] 2022 Feb 04; Vol. 128 (5), pp. 051101.
Publication Year :
2022

Abstract

We present an all-sky 90% confidence level upper limit on the cosmic flux of relativistic magnetic monopoles using 2886 days of IceCube data. The analysis was optimized for monopole speeds between 0.750c and 0.995c, without any explicit restriction on the monopole mass. We constrain the flux of relativistic cosmic magnetic monopoles to a level below 2.0×10^{-19}  cm^{-2} s^{-1} sr^{-1} over the majority of the targeted speed range. This result constitutes the most strict upper limit to date for magnetic monopoles with β≳0.8 and up to β∼0.995 and fills the gap between existing limits on the cosmic flux of nonrelativistic and ultrarelativistic magnetic monopoles.

Details

Language :
English
ISSN :
1079-7114
Volume :
128
Issue :
5
Database :
MEDLINE
Journal :
Physical review letters
Publication Type :
Academic Journal
Accession number :
35179913
Full Text :
https://doi.org/10.1103/PhysRevLett.128.051101