Updated Observing Scenarios and Multimessenger Implications for the International Gravitational-wave Networks O4 and O5

被引：22

作者：

Kiendrebeogo, R. Weizmann ^{[1
,2
,3
]}

Farah, Amanda M. ^{[4
]}

Foley, Emily M. ^{[3
,5
]}

Gray, Abigail ^{[3
]}

Kunert, Nina ^{[6
]}

Puecher, Anna ^{[7
,8
]}

Toivonen, Andrew ^{[3
]}

Vandenberg, R. Oliver ^{[3
]}

Anand, Shreya ^{[9
]}

Ahumada, Tomas ^{[9
]}

Karambelkar, Viraj ^{[9
]}

Coughlin, Michael W. ^{[3
]}

Dietrich, Tim ^{[6
,10
]}

Kam, S. Zacharie ^{[1
]}

Pang, Peter T. H. ^{[7
,8
]}

Singer, Leo P. ^{[11
]}

Sravan, Niharika ^{[12
]}

机构：

[1] Univ Joseph KI ZERBO, Lab Phys & Chim Environm, Ouagadougou, Burkina Faso

[2] Univ Cote dAzur, Artemis, Observ Cote dAzur, Blvd Observ, F-06304 Nice, France

[3] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA

[4] Univ Chicago, Dept Phys, Chicago, IL 60637 USA

[5] Wake Forest Univ, BS Phys, BA Math, Winston Salem, NC USA

[6] Univ Potsdam, Inst Phys & Astron, Theoret Astrophys, Haus 28, Karl Liebknecht Str 24-25, D-14476 Potsdam, Germany

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

[8] Univ Utrecht, Inst Gravitat & Subatom Phys GRASP, Princetonpl 1, NL-3584 CC Utrecht, Netherlands

[9] CALTECH, Cahill Ctr Astrophys, Pasadena, CA 91125 USA

[10] Albert Einstein Inst, Max Planck Inst Gravitat Phys, Muhlenberg 1, D-14476 Potsdam, Germany

[11] NASA, Astroparticle Phys Lab, Goddard Space Flight Ctr, Mail Code 661, Greenbelt, MD 20771 USA

[12] Drexel Univ, Dept Phys, Philadelphia, PA 19104 USA

来源：

ASTROPHYSICAL JOURNAL | 2023年 / 958卷 / 02期

基金：

美国国家科学基金会;

关键词：

NEUTRON-STAR MERGER; ZWICKY TRANSIENT FACILITY; EQUATION-OF-STATE; MULTI-MESSENGER OBSERVATIONS; R-PROCESS NUCLEOSYNTHESIS; GAMMA-RAY BURST; ELECTROMAGNETIC COUNTERPART; MASS-DISTRIBUTION; MAXIMUM MASS; FOLLOW-UP;

D O I：

10.3847/1538-4357/acfcb1

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

An advanced LIGO and Virgo's third observing run brought another binary neutron star merger (BNS) and the first neutron-star black hole mergers. While no confirmed kilonovae were identified in conjunction with any of these events, continued improvements of analyses surrounding GW170817 allow us to project constraints on the Hubble Constant (H 0), the Galactic enrichment from r-process nucleosynthesis, and ultra-dense matter possible from forthcoming events. Here, we describe the expected constraints based on the latest expected event rates from the international gravitational-wave network and analyses of GW170817. We show the expected detection rate of gravitational waves and their counterparts, as well as how sensitive potential constraints are to the observed numbers of counterparts. We intend this analysis as support for the community when creating scientifically driven electromagnetic follow-up proposals. During the next observing run O4, we predict an annual detection rate of electromagnetic counterparts from BNS of 0.43-0.26+0.58 ( 1.97-1.2+2.68 ) for the Zwicky Transient Facility (Rubin Observatory).

引用

页数：21

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