Neutrino rate predictions for FASER

被引：7

作者：

Abraham, Roshan Mammen ^{[1
]}

Anders, John ^{[2
]}

Antel, Claire ^{[3
]}

Ariga, Akitaka ^{[4
,5
]}

Ariga, Tomoko ^{[6
]}

Atkinson, Jeremy ^{[4
]}

Bernlochner, Florian U. ^{[7
]}

Boeckh, Tobias ^{[7
]}

Boyd, Jamie ^{[2
]}

Brenner, Lydia ^{[8
]}

Burger, Angela ^{[2
]}

Cadoux, Franck ^{[3
]}

Cardella, Roberto ^{[3
]}

Casper, David W. ^{[1
]}

Cavanagh, Charlotte ^{[9
]}

Chen, Xin ^{[10
]}

Coccaro, Andrea ^{[11
]}

Debieux, Stephane ^{[3
]}

D'Onofrio, Monica ^{[9
]}

Desai, Ansh ^{[12
]}

Dmitrievsky, Sergey

Eley, Sinead ^{[9
]}

Favre, Yannick ^{[3
]}

Fellers, Deion ^{[12
]}

Feng, Jonathan L. ^{[1
]}

Fenoglio, Carlo Alberto ^{[3
]}

Ferrere, Didier ^{[3
]}

Fieg, Max ^{[1
]}

Filali, Wissal ^{[7
]}

Gibson, Stephen ^{[13
]}

Gonzalez-Sevilla, Sergio ^{[3
]}

Gornushkin, Yuri

Gwilliam, Carl ^{[9
]}

Hayakawa, Daiki ^{[5
]}

Hsu, Shih-Chieh ^{[14
]}

Hu, Zhen ^{[10
]}

Iacobucci, Giuseppe ^{[3
]}

Inada, Tomohiro ^{[2
]}

Iodice, Luca ^{[3
]}

Jakobsen, Sune ^{[2
]}

Joos, Hans ^{[2
,15
]}

Kajomovitz, Enrique ^{[16
]}

Kawahara, Hiroaki ^{[6
]}

Keyken, Alex ^{[13
]}

Kling, Felix ^{[17
]}

Kock, Daniela ^{[12
]}

Kontaxakis, Pantelis ^{[3
]}

Kose, Umut ^{[18
]}

Kotitsa, Rafaella ^{[2
]}

Kuehn, Susanne ^{[2
]}

机构：

[1] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

[2] CERN, CH-1211 Geneva 23, Switzerland

[3] Univ Geneva, Dept Phys Nucl & Corpusculaire, CH-1211 Geneva 4, Switzerland

[4] Univ Bern, Albert Einstein Ctr Fundamental Phys, Lab High Energy Phys, Sidlerstr 5, CH-3012 Bern, Switzerland

[5] Chiba Univ, Dept Phys, 1-33 Yayoi Cho,Inage Ku, Chiba 2638522, Japan

[6] Kyushu Univ, Nishi Ku, Fukuoka 8190395, Japan

[7] Univ Bonn, Regina Pacis Weg 3, D-53113 Bonn, Germany

[8] Nikhef Natl Inst Subat Phys, Sci Pk 105, NL-1098 XG Amsterdam, Netherlands

[9] Univ Liverpool, Liverpool L69 3BX, Merseyside, England

[10] Tsinghua Univ, Dept Phys, Beijing, Peoples R China

[11] INFN, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy

[12] Univ Oregon, Eugene, OR 97403 USA

[13] Royal Holloway Univ London, Egham TW20 0EX, Surrey, England

[14] Univ Washington, Dept Phys, POB 351560, Seattle, WA 98195 USA

[15] Univ Gottingen, Phys Inst 2, Gottingen, Germany

[16] Technion Israel Inst Technol, Dept Phys & Astron, IL-32000 Haifa, Israel

[17] Deutsch Elektronen Synchrotron DESY, Notkestr 85, D-22607 Hamburg, Germany

[18] Swiss Fed Inst Technol, CH-8092 Zurich, Switzerland

[19] Weizmann Inst Sci, Dept Particle Phys & Astrophys, IL-76100 Rehovot, Israel

[20] Johannes Gutenberg Univ Mainz, Inst Phys, Mainz, Germany

[21] Univ Sussex, Dept Phys & Astron, Sussex House, Brighton BN1 9RH, E Sussex, England

[22] Nagoya Univ, Furo Cho,Chikusa Ku, Nagoya, Aichi 4648602, Japan

[23] Univ Manchester, Sch Phys & Astron, Schuster Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England

[24] Univ Napoli Federico II, Dipartimento Fis Ettore Pancini, Complesso Univ Monte S Angelo, I-80126 Naples, Italy

[25] KEK, Inst Particle & Nucl Studies, Tsukuba, Ibaraki 3050801, Japan

[26] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic

来源：

PHYSICAL REVIEW C | 2024年 / 110卷 / 01期

关键词：

PHYSICS FACILITY; CROSS-SECTIONS; MODEL;

D O I：

10.1103/PhysRevD.110.012009

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

The Forward Search Experiment (FASER) at CERN's Large Hadron Collider (LHC) has recently directly detected the first collider neutrinos. Neutrinos play an important role in all FASER analyses, either as signal or background, and it is therefore essential to understand the neutrino event rates. In this study, we update previous simulations and present prescriptions for theoretical predictions of neutrino fluxes and cross sections, together with their associated uncertainties. With these results, we discuss the potential for possible measurements that could be carried out in the coming years with the FASER neutrino data to be collected in LHC Run 3 and Run 4.

引用

页数：14