Constraints on Populations of Neutrino Sources from Searches in the Directions of IceCube Neutrino Alerts

Author:

Abbasi R.ORCID,Ackermann M.ORCID,Adams J.,Aggarwal N.,Aguilar J. A.ORCID,Ahlers M.ORCID,Alameddine J. M.ORCID,Alves A. A.ORCID,Amin N. M.,Andeen K.,Anderson T.,Anton G.ORCID,Argüelles C.ORCID,Ashida Y.,Athanasiadou S.,Axani S. N.ORCID,Bai X.ORCID,V. A. BalagopalORCID,Baricevic M.,Barwick S. W.ORCID,Basu V.ORCID,Bay R.,Beatty J. J.ORCID,Becker K.-H.,Tjus J. BeckerORCID,Beise J.ORCID,Bellenghi C.ORCID,Benda S.,BenZvi S.ORCID,Berley D.,Bernardini E.ORCID,Besson D. Z.ORCID,Binder G.,Bindig D.,Blaufuss E.ORCID,Blot S.ORCID,Bontempo F.,Book J. Y.ORCID,Borowka J.,Meneguolo C. BoscoloORCID,Böser S.ORCID,Botner O.ORCID,Böttcher J.,Bourbeau E.,Braun J.,Brinson B.,Brostean-Kaiser J.,Burley R. T.,Busse R. S.,Campana M. A.ORCID,Carnie-Bronca E. G.,Chen C.ORCID,Chen Z.ORCID,Chirkin D.ORCID,Choi K.,Clark B. A.ORCID,Classen L.,Coleman A.ORCID,Collin G. H.ORCID,Connolly A.,Conrad J. M.ORCID,Coppin P.ORCID,Correa P.ORCID,Countryman S.,Cowen D. F.ORCID,Cross R.ORCID,Dappen C.,Dave P.ORCID,De Clercq C.ORCID,DeLaunay J. J.ORCID,Delgado López D.ORCID,Dembinski H.ORCID,Deoskar K.,Desai A.ORCID,Desiati P.ORCID,de Vries K. D.ORCID,de Wasseige G.ORCID,DeYoung T.ORCID,Diaz A.ORCID,Díaz-Vélez J. C.ORCID,Dittmer M.,Dujmovic H.ORCID,DuVernois M. A.ORCID,Ehrhardt T.,Eller P.ORCID,Engel R.,Erpenbeck H.,Evans J.,Evenson P. A.ORCID,Fan K. L.ORCID,Fazely A. R.ORCID,Fedynitch A.ORCID,Feigl N.,Fiedlschuster S.,Fienberg A. T.ORCID,Finley C.ORCID,Fischer L.,Fox D.ORCID,Franckowiak A.ORCID,Friedman E.,Fritz A.,Fürst P.,Gaisser T. K.ORCID,Gallagher J.,Ganster E.ORCID,Garcia A.ORCID,Garrappa S.ORCID,Gerhardt L.,Ghadimi A.ORCID,Glaser C.ORCID,Glauch T.ORCID,Glüsenkamp T.ORCID,Goehlke N.,Gonzalez J. G.,Goswami S.ORCID,Grant D.,Gray S. J.ORCID,Grégoire T.ORCID,Griswold S.ORCID,Günther C.,Gutjahr P.ORCID,Haack C.,Hallgren A.ORCID,Halliday R.,Halve L.ORCID,Halzen F.ORCID,Hamdaoui H.,Minh M. Ha,Hanson K.,Hardin J.,Harnisch A. A.,Hatch P.,Haungs A.ORCID,Helbing K.ORCID,Hellrung J.,Henningsen F.ORCID,Heuermann L.,Hickford S.,Hidvegi A.,Hill C.ORCID,Hill G. C.,Hoffman K. D.,Hoshina K.,Hou W.,Huber T.ORCID,Hultqvist K.ORCID,Hünnefeld M.,Hussain R.,Hymon K.,In S.,Iovine N.ORCID,Ishihara A.,Jansson M.,Japaridze G. S.ORCID,Jeong M.,Jin M.ORCID,Jones B. J. P.ORCID,Kang D.ORCID,Kang W.ORCID,Kang X.,Kappes A.ORCID,Kappesser D.,Kardum L.,Karg T.ORCID,Karl M.ORCID,Karle A.ORCID,Katz U.ORCID,Kauer M.ORCID,Kelley J. L.ORCID,Kheirandish A.ORCID,Kin K.,Kiryluk J.ORCID,Klein S. R.ORCID,Kochocki A.ORCID,Koirala R.ORCID,Kolanoski H.ORCID,Kontrimas T.,Köpke L.ORCID,Kopper C.ORCID,Koskinen D. J.ORCID,Koundal P.ORCID,Kovacevich M.ORCID,Kowalski M.ORCID,Kozynets T.,Krupczak E.,Kun E.ORCID,Kurahashi N.ORCID,Lad N.,Lagunas Gualda C.ORCID,Larson M. J.ORCID,Lauber F.ORCID,Lazar J. P.ORCID,Lee J. W.ORCID,Leonard K.ORCID,Leszczyńska A.ORCID,Lincetto M.,Liu Q. R.ORCID,Liubarska M.,Lohfink E.ORCID,Love C.,Mariscal C. J. Lozano,Lu L.ORCID,Lucarelli F.ORCID,Ludwig A.ORCID,Luszczak W.ORCID,Lyu Y.ORCID,Ma W. Y.ORCID,Madsen J.ORCID,Mahn K. B. M.,Makino Y.,Mancina S.,Sainte W. Marie,Mariş I. C.ORCID,Marka S.,Marka Z.,Marsee M.,Martinez-Soler I.,Maruyama R.ORCID,McElroy T.,McNally F.ORCID,Mead J. V.,Meagher K.ORCID,Mechbal S.,Medina A.,Meier M.ORCID,Meighen-Berger S.ORCID,Merckx Y.,Micallef J.,Mockler D.,Montaruli T.ORCID,Moore R. W.ORCID,Morse R.,Moulai M.ORCID,Mukherjee T.,Naab R.ORCID,Nagai R.ORCID,Naumann U.,Nayerhoda A.ORCID,Necker J.ORCID,Neumann M.,Niederhausen H.ORCID,Nisa M. U.ORCID,Noell A.,Nowicki S. C.ORCID,Pollmann A. ObertackeORCID,Oehler M.,Oeyen B.ORCID,Olivas A.,Orsoe R.,Osborn J.,O’Sullivan E.ORCID,Pandya H.ORCID,Pankova D. V.,Park N.ORCID,Parker G. K.,Paudel E. N.ORCID,Paul L.,de los Heros C. PérezORCID,Peters L.,Peterson J.ORCID,Philippen S.,Pieper S.,Pizzuto A.ORCID,Plum M.ORCID,Popovych Y.,Porcelli A.ORCID,Prado Rodriguez M.,Pries B.ORCID,Procter-Murphy R.,Przybylski G. T.,Raab C.ORCID,Rack-Helleis J.,Rameez M.ORCID,Rawlins K.,Rechav Z.,Rehman A.ORCID,Reichherzer P.,Renzi G.,Resconi E.ORCID,Reusch S.ORCID,Rhode W.ORCID,Richman M.,Riedel B.ORCID,Roberts E. J.,Robertson S.,Rodan S.,Roellinghoff G.,Rongen M.ORCID,Rott C.ORCID,Ruhe T.,Ruohan L.,Ryckbosch D.ORCID,Rysewyk Cantu D.ORCID,Safa I.ORCID,Saffer J.,Salazar-Gallegos D.ORCID,Sampathkumar P.,Sanchez Herrera S. E.,Sandrock A.ORCID,Santander M.ORCID,Sarkar S.ORCID,Sarkar S.ORCID,Savelberg J.,Schaufel M.,Schieler H.ORCID,Schindler S.ORCID,Schlueter B.,Schmidt T.,Schneider J.ORCID,Schröder F. G.ORCID,Schumacher L.,Schwefer G.ORCID,Sclafani S.ORCID,Seunarine S.,Sharma A.ORCID,Shefali S.,Shimizu N.,Silva M.ORCID,Skrzypek B.,Smithers B.ORCID,Snihur R.,Soedingrekso J.ORCID,Søgaard A.,Soldin D.ORCID,Spannfellner C.,Spiczak G. M.ORCID,Spiering C.ORCID,Stamatikos M.,Stanev T.,Stein R.ORCID,Stezelberger T.ORCID,Stürwald T.,Stuttard T.ORCID,Sullivan G. W.ORCID,Taboada I.ORCID,Ter-Antonyan S.ORCID,Thompson W. G.ORCID,Thwaites J.,Tilav S.,Tollefson K.ORCID,Tönnis C.,Toscano S.ORCID,Tosi D.,Trettin A.ORCID,Tung C. F.ORCID,Turcotte R.,Twagirayezu J. P.,Ty B.,Unland Elorrieta M. A.ORCID,Upshaw K.,Valtonen-Mattila N.ORCID,Vandenbroucke J.ORCID,van Eijndhoven N.ORCID,Vannerom D.,van Santen J.ORCID,Vara J.,Veitch-Michaelis J.,Verpoest S.ORCID,Veske D.,Walck C.ORCID,Wang W.,Watson T. B.ORCID,Weaver C.ORCID,Weigel P.,Weindl A.,Weldert J.ORCID,Wendt C.ORCID,Werthebach J.,Weyrauch M.,Whitehorn N.ORCID,Wiebusch C. H.ORCID,Willey N.,Williams D. R.,Wolf M.ORCID,Wrede G.,Wulff J.,Xu X. W.,Yanez J. P.,Yildizci E.,Yoshida S.ORCID,Yu S.,Yuan T.ORCID,Zhang Z.ORCID,Zhelnin P.,

Abstract

Abstract Beginning in 2016, the IceCube Neutrino Observatory has sent out alerts in real time containing the information of high-energy (E ≳ 100 TeV) neutrino candidate events with moderate to high (≳30%) probability of astrophysical origin. In this work, we use a recent catalog of such alert events, which, in addition to events announced in real time, includes events that were identified retroactively and covers the time period of 2011–2020. We also search for additional, lower-energy neutrinos from the arrival directions of these IceCube alerts. We show how performing such an analysis can constrain the contribution of rare populations of cosmic neutrino sources to the diffuse astrophysical neutrino flux. After searching for neutrino emission coincident with these alert events on various timescales, we find no significant evidence of either minute-scale or day-scale transient neutrino emission or of steady neutrino emission in the direction of these alert events. This study also shows how numerous a population of neutrino sources has to be to account for the complete astrophysical neutrino flux. Assuming that sources have the same luminosity, an E −2.5 neutrino spectrum, and number densities that follow star formation rates, the population of sources has to be more numerous than 7 × 10−9 Mpc−3. This number changes to 3 × 10−7 Mpc−3 if number densities instead have no cosmic evolution.

Funder

National Science Foundation

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 3 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. On the “Loose” Constraint from IceCube Neutrino Nondetection of GRB 230307A;The Astrophysical Journal;2023-11-20

2. IceCat-1: The IceCube Event Catalog of Alert Tracks;The Astrophysical Journal Supplement Series;2023-11-01

3. Neutrino flares of radio blazars observed from TeV to PeV;Monthly Notices of the Royal Astronomical Society: Letters;2023-09-26

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3