From One to Many: Statistical Gravitational-Wave Astrophysics and Cosmology

从一到多：统计引力波天体物理学和宇宙学

• 批准号: 2110507
• 负责人: Daniel Holz
• 金额: $ 45万
• 依托单位: University of Chicago
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2021
• 资助国家: 美国
• 起止时间: 2021-07-15 至 2024-06-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2110507&HistoricalAwards=false
• 关键词: Many; Statistical; Gravitational; Wave; Astrophysics

The 2015 discovery of gravitational waves, ripples in the fabric of space and time, electrified the scientific community and was awarded the Nobel Prize. Scientists are now routinely detecting gravitational waves from the collisions of neutron stars and/or black holes. A catalog of 50 such mergers has been assembled, with hundreds more expected in the coming years. This project will analyze this growing catalog, and determine the distribution of properties such as the mass and spin of the black holes as well as their distances. By analyzing all of this information, it is possible to infer important insights about how the black holes were formed in the first place. And the formation of black holes is particularly fascinating because it relates to the deaths of stars, since black holes are thought to be formed from dying stars. Even more interesting, the recent detections of big black holes, some of them well over 50 times the mass of our Sun, are related to the deaths of very big stars—these are specifically thought to be some of the earliest and most pristine stars. In short, by studying black hole collisions, this study will learn about the first stars in the Universe, and therefore the process by which the Universe makes stars, galaxies, the elements, and eventually, the Earth and everything on it. In addition to producing important and novel science, this proposal will also convey some of the beauty and excitement of the field to the broader public, ranging from primary school students through to senior citizens.The burgeoning catalog of events enables an entirely new approach to elucidating science from gravitational-wave sources: statistical inference from the detected population of gravitational events. This project will advance the field of gravitational-wave population astrophysics by building the tools and analysis pipelines to answer some of the most exciting astrophysical questions related to LIGO sources. Specific research projects will include characterizing mass gaps, spin and mass ratio distributions, and the redshift evolution of the detected population. These results will inform constraints on the astrophysical formation channels of binary systems. For small samples, every event is in some sense an “outlier”; as the population grows, the PI will explore the critical astrophysical relevance of outliers and sub-populations. In addition, the PI will explore population constraints on the neutron star equation of state, and further develop a novel probe of binary formation physics and astrophysics through the binary-host connection. The study will continue to develop standard sirens as uniquely clean and powerful cosmological probes, including extending counterpart and statistical standard sirens constraints, and refining pipelines and preparing for the possibility of exciting standard siren sources in the LIGO/Virgo O4 observational science run. Work will also include further development of novel approaches to standard siren science, including the exploration of mass-gap cosmology. The project will use the upper and lower edges of the mass distribution as observational “features” to provide independent constraints of the expansion history of the universe to very high redshift. As the number of gravitational-wave detections continues to grow by leaps and bounds, statistical characterization of the events will provide important insights, and this work will help pave the way for population gravitational-wave astrophysics and cosmology.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

2015年引力波的发现，空间和时间结构中的涟漪，使科学界感到震惊，并被授予诺贝尔奖。科学家们现在经常探测来自中子星和/或黑洞碰撞的引力波。一份包含50起此类合并的目录已经汇总，预计未来几年还会有数百起。该项目将分析这一不断增长的目录，并确定黑洞的质量和自旋以及它们的距离等属性的分布。通过分析所有这些信息，可以推断出有关黑洞最初是如何形成的重要见解。黑洞的形成特别吸引人，因为它与恒星的死亡有关，因为黑洞被认为是由垂死的恒星形成的。更有趣的是，最近发现的大黑洞，其中一些质量超过太阳的50倍，与非常大的恒星的死亡有关-这些被认为是最早和最原始的恒星。简而言之，通过研究黑洞碰撞，这项研究将了解宇宙中的第一批恒星，从而了解宇宙形成恒星、星系、元素的过程，最终了解地球及其上的一切。除了产生重要而新颖的科学，这项提议还将向更广泛的公众传达该领域的一些美丽和兴奋之处，从小学生到老年人。迅速发展的事件目录使一种全新的方法能够从引力波源阐明科学：从检测到的引力事件群体中进行统计推断。该项目将通过构建工具和分析管道来推进引力波布居天体物理学领域，以回答与LIGO源相关的一些最令人兴奋的天体物理学问题。具体的研究项目将包括表征质量间隙，自旋和质量比分布，以及检测到的人口的红移演变。这些结果将告知约束的天体物理形成通道的二元系统。对于小样本，每个事件在某种意义上都是一个“离群值”;随着人口的增长，PI将探索离群值和子人口的关键天体物理相关性。此外，PI将探索中子星星状态方程的布居约束，并通过双星-宿主连接进一步开发双星形成物理和天体物理的新探测器。该研究将继续开发标准警报器作为独特的清洁和强大的宇宙学探测器，包括扩展对应和统计标准警报器约束，并完善管道，为LIGO/Virgo O 4观测科学运行中激发标准警报器源的可能性做准备。工作还将包括进一步开发标准海妖科学的新方法，包括探索质量间隙宇宙学。该项目将使用质量分布的上下边缘作为观测“特征”，以提供对宇宙膨胀历史的独立约束，使其具有非常高的红移。随着引力波探测数量的持续跳跃式增长，事件的统计特征将提供重要的见解，这项工作将有助于为人口引力波天体物理学和宇宙学铺平道路。该奖项反映了NSF的法定使命，并通过使用基金会的智力价值和更广泛的影响审查标准进行评估，被认为值得支持。

项目成果

Search for Subsolar-Mass Binaries in the First Half of Advanced LIGO’s and Advanced Virgo’s Third Observing Run

在 Advanced LIGO 和 Advanced Virgo 第三次观测运行的前半段中搜索太阳质量以下的双星

• DOI: 10.1103/physrevlett.129.061104
• 发表时间: 2022
• 期刊: Physical Review Letters
• 影响因子: 8.6
• 作者: Abbott, R.;Abbott, T. D.;Acernese, F.;Ackley, K.;Adams, C.;Adhikari, N.;Adhikari, R. X.;Adya, V. B.;Affeldt, C.;Agarwal, D.
• 通讯作者: Agarwal, D.

(An)isotropy measurement with gravitational wave observations

• DOI: 10.1103/physrevd.107.043016
• 发表时间: 2022-07
• 期刊: Physical Review D
• 影响因子: 5
• 作者: R. Essick;W. Farr;M. Fishbach;D. Holz;E. Katsavounidis

All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 data

• DOI: 10.1103/physrevd.106.102008
• 发表时间: 2022-01
• 期刊: Physical Review D
• 影响因子: 5
• 作者: The Ligo Scientific Collaboration;The Virgo Collaboration;T. Abbott;H. Abe;F. Acernese;K. Ackley;N. Adhikari;R. Adhikari;V. K. Adkins;V. Adya;C. Affeldt;D. Agarwal;M. Agathos;K. Agatsuma;N. Aggarwal;O. Aguiar;L. Aiello;A. Ain;P. Ajith;T. Akutsu;S. Albanesi;R. Alfaidi;A. Allocca;P. Altin;A. Amato;C. Anand;S. Anand;A. Ananyeva;S. Anderson;W. Anderson;M. Ando;T. Andrade;N. Andrés;M. Andr'es-Carcasona;T. Andri'c;S. Angelova;S. Ansoldi;J. Antelis;S. Antier;T. Apostolatos;E. Z. Appavuravther;S. Appert;S. Apple;K. Arai;A. Araya;M. Araya;J. Areeda;M. Arène;N. Aritomi;N. Arnaud;M. Arogeti;S. Aronson;H. Asada;Y. Asali;G. Ashton;Y. Aso;M. Assiduo;S. D. Melo;S. Aston;P. Astone;F. Aubin;K. AultONeal;C. Austin;S. Babak;F. Badaracco;M. Bader;C. Badger;S. Bae;Y. Bae;A. Baer;S. Bagnasco;Y. Bai;J. Baird;R. Bajpai;T. Baka;M. Ball;G. Ballardin;S. Ballmer;A. Balsamo;G. Baltus;S. Banagiri;B. Banerjee;D. Bankar;J. Barayoga;C. Barbieri;B. Barish;D. Barker;P. Barneo;F. Barone;B. Barr;L. Barsotti;M. Barsuglia;D. Barta;J. Bartlett;M. Barton;I. Bartos;S. Basak;R. Bassiri;A. Basti;M. Bawaj;J. Bayley;M. Bazzan;B. Becher;B. B'ecsy;V. Bedakihale;F. Beirnaert;M. Bejger;I. Belahcene;V. Benedetto;D. Beniwal;M. Benjamin;T. Bennett;J. Bentley;M. BenYaala;S. Bera;M. Berbel;F. Bergamin;B. Berger;S. Bernuzzi;D. Bersanetti;A. Bertolini;J. Betzwieser;D. Beveridge;R. Bhandare;A. Bhandari;U. Bhardwaj;R. Bhatt;D. Bhattacharjee;S. Bhaumik;A. Bianchi;I. Bilenko;G. Billingsley;S. Bini;R. Birney;O. Birnholtz;S. Biscans;M. Bischi;S. Biscoveanu;A. Bisht;B. Biswas;M. Bitossi;M. Bizouard;J. Blackburn;C. Blair;D. Blair;R. Blair;F. Bobba;N. Bode;M. Boer;G. Bogaert;M. Boldrini;G. N. Bolingbroke;L. D. Bonavena;F. Bondu;E. Bonilla;R. Bonnand;P. Booker;B. A. Boom;R. Bork;V. Boschi;N. Bose;S. Bose;V. Bossilkov;V. Boudart;Y. Bouffanais;A. Bozzi;C. Bradaschia;P. Brady;A. Bramley;A. Branch;M. Branchesi;J. Brau;M. Breschi;T. Briant;J. Briggs;A. Brillet;M. Brinkmann;P. Brockill;A. Brooks;J. Brooks;D. Brown;S. Brunett;G. Bruno;R. Bruntz;J. Bryant;F. Bucci;T. Bulik;H. Bulten;A. Buonanno;K. Burtnyk;R. Buscicchio;D. Buskulic;C. Buy;R. Byer;G. Davies;G. Cabras;R. Cabrita;L. Cadonati;M. Caesar;G. Cagnoli;C. Cahillane;J. C. Bustillo;J. Callaghan;T. Callister;E. Calloni;J. Cameron;J. Camp;M. Canepa;S. Canevarolo;M. Cannavacciuolo;K. Cannon;H. Cao;Z. Cao;E. Capocasa;E. Capote;G. Carapella;F. Carbognani;M. Carlassara;J. Carlin;M. Carney;M. Carpinelli;G. Carrillo;Gregorio Carullo;T. Carver;J. C. Diaz;C. Casentini;G. Castaldi;S. Caudill;M. Cavaglià;F. Cavalier;R. Cavalieri;G. Cella;P. Cerd'a-Dur'an;E. Cesarini;W. Chaibi;S. Subrahmanya;E. Champion;C. Chan;C. Chan;C. Chan;K. Chan;M. Chan;K. Chandra;I. Chang;P. Chanial;S. Chao;C. Chapman-Bird;P. Charlton;E. Chase;É. Chassande-Mottin;C. Chatterjee;D. Chatterjee;D. Chatterjee;M. Chaturvedi;S. Chaty;C. Chen;D. Chen;H. Chen;J. Chen;K. Chen;X. Chen;Y. Chen;Y.-R. Chen;Z. Chen;H. Cheng;C. Cheong;H. Cheung;H. Chia;F. Chiadini;C. Chiang;G. Chiarini;R. Chierici;A. Chincarini;M. Chiofalo;A. Chiummo;Rupesh Kumar Choudhary;S. Choudhary;N. Christensen;Q. Chu;Y. Chu;S. Chua;K. Chung;G. Ciani;P. Ciecieląg;M. Cie'slar;M. Cifaldi;A. Ciobanu;R. Ciolfi;F. Cipriano;F. Clara;J. Clark;P. Clearwater;S. Clesse;F. Cleva;E. Coccia;E. Codazzo;P. Cohadon;D. Cohen;M. Colleoni;C. Collette;A. Colombo;M. Colpi;C. Compton;M. Constancio;L. Conti;S. Cooper;P. Corban;T. Corbitt;I. Cordero-Carri'on;S. Corezzi;K. Corley;N. Cornish;D. Corre;A. Corsi;S. Cortese;C. Costa;R. Cotesta;R. Cottingham;M. Coughlin;J. Coulon;S. Countryman;B. Cousins;P. Couvares;D. Coward;M. Cowart;D. Coyne;R. Coyne;J. Creighton;T. Creighton;A. Criswell;M. Croquette;S. Crowder;J. Cudell;T. Cullen;A. Cumming;R. Cummings;L. Cunningham;E. Cuoco;M. Curyło;P. Dabadie;T. D. Canton;S. Dall’Osso;G. D'alya;A. Dana;Beatrice D'Angelo;S. Danilishin;S. D’Antonio;K. Danzmann;C. Darsow-Fromm;A. Dasgupta;L. Datrier;Sayak Datta;S. Datta;V. Dattilo;I. Dave;M. Davier;D. Davis;M. Davis;E. Daw;R. Dean;D. DeBra;M. Deenadayalan;J. Degallaix;M. D. Laurentis;S. Del'eglise;V. D. Favero;F. D. Lillo;N. D. Lillo;D. Dell’Aquila;W. D. Pozzo;L. DeMarchi;F. Matteis;V. D'Emilio;N. Demos;T. Dent;A. Depasse;R. Pietri;R. Rosa;C. Rossi;R. DeSalvo;R. D. Simone;S. Dhurandhar;M. D'iaz;M. D. Cesare;N. Didio;T. Dietrich;L. Fiore;C. D. Fronzo;C. Giorgio;F. D. Giovanni;M. Giovanni;T. D. Girolamo;A. Lieto;A. D. Michele;B. Ding;S. D. Pace;I. Palma;F. Renzo;A. K. Divakarla;A. Dmitriev;Zoheyr Doctor;L. Donahue;L. D’Onofrio;F. Donovan;K. Dooley;S. Doravari;O. Dorosh;M. Drago;J. Driggers;Y. Drori;J. Ducoin;P. Dupej;U. Dupletsa;O. Durante;D. D’Urso;P. Duverne;S. Dwyer;C. Eassa;P. Easter;M. Ebersold;T. Eckhardt;G. Eddolls;B. Edelman;T. Edo;O. Edy;A. Effler;S. Eguchi;J. Eichholz;S. Eikenberry;M. Eisenmann;R. Eisenstein;A. Ejlli;E. Engelby;Y. Enomoto;L. Errico;R. Essick;H. Estell'es;D. Estevez;Z. Etienne;T. Etzel;M. Evans;T. Evans;T. Evstafyeva;B. Ewing;F. Fabrizi;F. Faedi;V. Fafone;H. Fair;S. Fairhurst;P. Fan;A. M. Farah;S. Farinon;B. Farr;W. Farr;E. Fauchon-Jones;G. Favaro;Marc Favata;M. Fays;M. Fazio;J. Feicht;M. Fejer;E. Fenyvesi;D. Ferguson;Á. Fernández-Galiana;I. Ferrante;T. A. Ferreira;F. Fidecaro;P. Figura;A. Fiori;I. Fiori;M. Fishbach;R. Fisher;R. Fittipaldi;V. Fiumara;R. Flaminio;E. Floden;H. Fong;J. Font;B. Fornal;P. Forsyth;A. Franke;S. Frasca;F. Frasconi;J. Freed;Z. Frei;A. Freise;O. Freitas;R. Frey;P. Fritschel;V. Frolov;G. G. Fronz'e-G.;Y. Fujii;Y. Fujikawa;Y. Fujimoto;P. Fulda;M. Fyffe;H. Gabbard;B. Gadre;J. Gair;J. Gais;S. Galaudage;R. Gamba;D. Ganapathy;A. Ganguly;D. Gao;S. Gaonkar;B. Garaventa;C. N'unez;C. Garc'ia-Quir'os;F. Garufi;B. Gateley;V. Gayathri;G. Ge;G. Gemme;A. Gennai;J. George;O. Gerberding;L. Gergely;P. Gewecke;S. Ghonge;A. Ghosh;A. Ghosh;Shaon Ghosh;Shrobana Ghosh;T. Ghosh;B. Giacomazzo;L. Giacoppo;J. Giaime;K. Giardina;D. Gibson;C. Gier;M. Giesler;P. Giri;F. Gissi;S. Gkaitatzis;J. Glanzer;A. Gleckl;P. Godwin;E. Goetz;R. Goetz;N. Gohlke;J. Golomb;B. Goncharov;G. Gonz'alez;M. Gosselin;R. Gouaty;D. Gould;S. Goyal;B. Grace;A. Grado;V. Graham;M. Granata;V. Granata;A. Grant;S. Gras;P. Grassia;C. Gray;R. Gray;G. Greco;A. Green;R. Green;A. Gretarsson;E. Gretarsson;D. Griffith;W. Griffiths;H. L. Griggs;G. Grignani;A. Grimaldi;E. Grimes;S. Grimm;H. Grote;S. Grunewald;P. Gruning;A. Gruson;D. Guerra;G. Guidi;A. R. Guimaraes;G. Guix'e;H. Gulati;A. Gunny;H.-K. Guo;Y. Guo;Anchal Gupta;Anuradha Gupta;I. M. Gupta;P. Gupta;S. Gupta;R. Gustafson;F. Guzmán;S. Ha;I. Hadiputrawan;L. Haegel;S. Haino;O. Halim;E. Hall;E. Hamilton;G. Hammond;W. Han;M. Haney;J. Hanks;C. Hanna;M. Hannam;O. Hannuksela;H. Hansen;T. Hansen;J. Hanson;T. Harder;K. Haris;J. Harms;G. Harry;I. Harry;D. Hartwig;K. Hasegawa;B. Haskell;C. Haster;J. S. Hathaway;K. Hattori;K. Haughian;H. Hayakawa;K. Hayama;F. Hayes;J. Healy;A. Heidmann;A. Heidt;M. Heintze;J. Heinze;J. Heinzel;H. Heitmann;F. Hellman;P. Hello;A. Helmling-Cornell;G. Hemming;M. Hendry;I. Heng;E. Hennes;J. Hennig;M. Hennig;C. Henshaw;A. Hernandez;F. Vivanco;M. Heurs;A. Hewitt;S. Higginbotham;S. Hild;P. Hill;Y. Himemoto;A. Hines;N. Hirata;C. Hirose;T. Ho;S. Hochheim;D. Hofman;J. Hohmann;D. Holcomb;N. Holland;I. J. Hollows;Z. J. Holmes;K. Holt;D. Holz;Q. Hong;J. Hough;S. Hourihane;E. Howell;C. Hoy;D. Hoyland;A. Hreibi;B. Hsieh;H. Hsieh;C. Hsiung;Y. Hsu;H. Huang;P. Huang;Y. Huang;Y. Huang;Yiting Huang;Yiwen Huang;M. Hubner;A. Huddart;B. Hughey;D. Hui;V. Hui;S. Husa;S. Huttner;R. Huxford;T. Huynh--Dinh-T.-Huynh--Dinh-1381195806;S. Ide;B. Idzkowski;A. Iess;K. Inayoshi;Y. Inoue;P. Iosif;M. Isi;K. Isleif;K. Ito;Y. Itoh;B. Iyer;V. JaberianHamedan;T. Jacqmin;P. Jacquet;S. Jadhav;S. Jadhav;T. Jain;A. James;A. Jan;K. Jani;J. Janquart;K. Janssens;N. Janthalur;P. Jaranowski;D. Jariwala;R. Jaume;A. Jenkins;K. Jenner;C. Jeon;W. Jia;J. Jiang;H. Jin;G. Johns;R. Johnston;A. Jones;D. Jones;P. Jones;R. Jones;P. Joshi;L. Ju;A. Jue;P. Jung;K. Jung;J. Junker;V. Juste;K. Kaihotsu;T. Kajita;M. Kakizaki;C. Kalaghatgi;V. Kalogera;B. Kamai;M. Kamiizumi;N. Kanda;S. Kandhasamy;G. Kang;J. Kanner;Y. Kao;S. Kapadia;D. Kapasi;C. Karathanasis;S. Karki;R. Kashyap;M. Kasprzack;W. Kastaun;T. Kato;S. Katsanevas;E. Katsavounidis;W. Katzman;T. Kaur;K. Kawabe;K. Kawaguchi;F. K'ef'elian;D. Keitel;J. Key;S. Khadka;F. Khalili;S. Khan;T. Khanam;E. Khazanov;N. Khetan;M. Khursheed;N. Kijbunchoo;A. Kim;C. Kim;J. Kim;J. Kim;K. Kim;W. Kim;Y. Kim;C. Kimball;N. Kimura;M. Kinley-Hanlon;R. Kirchhoff;J. Kissel;S. Klimenko;T. Klinger;A. Knee;T. Knowles;N. Knust;E. Knyazev;Y. Kobayashi;P. Koch;G. Koekoek;K. Kohri;K. Kokeyama;S. Koley;P. Kolitsidou;M. Kolstein;K. Komori;V. Kondrashov;A. Kong;A. Kontos;N. Koper;M. Korobko;M. Kovalam;N. Koyama;D. Kozak;C. Kozakai;V. Kringel;A. Kr'olak;G. Kuehn;F. Kuei;P. Kuijer;S. Kulkarni;A. Kumar;Prayush Kumar;Rahul Kumar;Rakesh Kumar;J. Kume;K. Kuns;Y. Kuromiya;S. Kuroyanagi;K. Kwak;G. LaCaille;P. Lagabbe;D. Laghi;É. Lalande;M. Lalleman;T. Lam;A. Lamberts;M. Landry;B. Lane;R. Lang;J. Lange;B. Lantz;I. L. Rosa;A. Lartaux-Vollard;P. Lasky;M. Laxen;A. Lazzarini;C. Lazzaro;P. Leaci;S. Leavey;S. LeBohec;Y. Lecoeuche;E. Lee;H. Lee;H. W. Lee;K. Lee;Ray-Kuang Lee;I. Legred;J. Lehmann;A. Lemaitre;M. Lenti;M. Leonardi;E. Leonova;N. Leroy;N. Letendre;C. Lévesque;Y. Levin;J. Leviton;K. Leyde;A. Li;B. Li;J. Li;K. Li;P. Li;T. G. F. Li;X. Li;C.Y. Lin;E. Lin;F. Lin;F. Lin;H. Lin;L. Lin;F. Linde;S. Linker;J. Linley;T. Littenberg;G. Liu;J. Liu;K. Liu;X. Liu;F. Llamas;R. K. Lo;T. Lo;L. London;A. Longo;D. Lopez;M. Portilla;M. Lorenzini;V. Loriette;M. Lormand;G. Losurdo;T. Lott;J. Lough;C. Lousto;G. Lovelace;J. F. Lucaccioni;H. Luck;D. Lumaca;A. Lundgren;L. Luo;J. Lynam;M. Ma'arif;R. Macas;J. Machtinger;M. Macinnis;D. Macleod;I. MacMillan;A. Macquet;I. M. Hernandez;C. Magazzù;R. Magee;R. Maggiore;M. Magnozzi;S. Mahesh;E. Majorana;I. Maksimovic;S. Maliakal;A. Malik;N. Man;V. Mandic;V. Mangano;G. Mansell;M. Manske;M. Mantovani;M. Mapelli;F. Marchesoni;D. Pina;F. Marion;Z. Mark;S. M'arka;Z. M'arka;C. Markakis;A. Markosyan;A. Markowitz;E. Maros;A. Marquina;S. Marsat;F. Martelli;I. Martin;R. Martin;M. Martínez;V. Martínez;V. Martínez;K. Martinovic;D. Martynov;E. J. Marx;H. Masalehdan;K. Mason;E. Massera;A. Masserot;M. Masso-Reid;S. Mastrogiovanni;A. Matas;M. Mateu-Lucena;F. Matichard;M. Matiushechkina;N. Mavalvala;J. McCann;R. Mccarthy;D. McClelland;P. McClincy;S. Mccormick;L. McCuller;G. McGhee;S. Mcguire;C. McIsaac;J. McIver;T. McRae;S. McWilliams;D. Meacher;M. Mehmet;A. Mehta;Q. Meijer;A. Melatos;D. Melchor;G. Mendell;A. Menéndez-Vázquez;C. Menoni;R. Mercer;L. Mereni;K. Merfeld;E. Merilh;J. D. Merritt;M. Merzougui;S. Meshkov;C. Messenger;C. Messick;P. Meyers;F. Meylahn;A. Mhaske;A. Miani;H. Miao;I. Michaloliakos;C. Michel;Y. Michimura;H. Middleton;D. Mihaylov;L. Milano;A. Miller;A. Miller;B. Miller;M. Millhouse;J. Mills;E. Milotti;Y. Minenkov;N. Mio;L. Mir;M. Miravet-Ten'es;A. Mishkin;C. Mishra;T. Mishra;T. Mistry;S. Mitra;V. Mitrofanov;G. Mitselmakher;R. Mittleman;O. Miyakawa;K. Miyo;S. Miyoki;G. Mo;L. M. Modafferi;E. Moguel;K. Mogushi;S. Mohapatra;S. Mohite;I. Molina;M. Molina-Ruiz;M. Mondin;M. Montani;C. Moore;J. Moragues;D. Moraru;F. Morawski;A. More;C. Moreno;G. Moreno;Y. Mori;S. Morisaki;N. Morisue;Y. Moriwaki;B. Mours;C. Mow-Lowry;S. Mozzon;F. Muciaccia;A. Mukherjee;D. Mukherjee;S. Mukherjee;S. Mukherjee;S. Mukherjee;N. Mukund;A. Mullavey;J. Munch;E. Muniz;P. Murray;R. Musenich;S. Muusse;S. Nadji;K. Nagano;A. Nagar;K. Nakamura;H. Nakano;M. Nakano;Y. Nakayama;V. Napolano;I. Nardecchia;T. Narikawa;H. Narola;L. Naticchioni;B. Nayak;R. Nayak;B. Neil;J. Neilson;A. Nelson;T. Nelson;M. Nery;P. Neubauer;A. Neunzert;K. Ng;S. Ng;C. Nguyen;P. Nguyen;T. Nguyen;L. Quynh;J. Ni;W. Ni;S. Nichols;T. Nishimoto;A. Nishizawa;S. Nissanke;E. Nitoglia;F. Nocera;M. Norman;C. North;S. Nozaki;G. Nurbek;L. Nuttall;Y. Obayashi;J. Oberling;B. O'Brien;J. O'Dell;E. Oelker;W. Ogaki;G. Oganesyan;J. Oh;K. Oh;S. Oh;M. Ohashi;T. Ohashi;M. Ohkawa;F. Ohme;H. Ohta;M. A. Okada;Y. Okutani;C. Olivetto;K. Oohara;R. Oram;B. O'reilly;R. Ormiston;N. Ormsby;R. O’Shaughnessy;É. O’Shea;S. Oshino;S. Ossokine;C. Osthelder;S. Otabe;D. Ottaway;H. Overmier;A. Pace;G. Pagano;R. Pagano;M. Page;G. Pagliaroli;A. Pai;S. Pai;S. Pal;J. R. Palamos;O. Palashov;C. Palomba;H. Pan;K. Pan;P. Panda;P. T. Pang;C. Pankow;F. Pannarale;B. Pant;F. Panther;F. Paoletti;A. Paoli;A. Paolone;George Pappas;A. Parisi;H. Park;J. Park;W. Parker;D. Pascucci;A. Pasqualetti;R. Passaquieti;D. Passuello;M. Patel;M. Pathak;B. Patricelli;A. S. Patron;S. Paul;E. Payne;M. Pedraza;R. Pedurand;M. Pegoraro;A. Pele;F. Arellano;S. Penano;S. Penn;A. Perego;A. Pereira;T. Pereira;C. Perez;C. P'erigois;C. Perkins;A. Perreca;S. Perriès;D. Pesios;J. Petermann;D. Petterson;H. Pfeiffer;H. Pham;K. A. Pham;K. S. Phukon;H. Phurailatpam;O. Piccinni;M. Pichot;M. Piendibene;F. Piergiovanni;L. Pierini;V. Pierro;G. Pillant;M. Pillas;F. Pilo;L. Pinard;C. Pineda-Bosque;I. Pinto;M. Pinto;B. Piotrzkowski;K. Piotrzkowski;M. Pirello;A. Pisarski;M. Pitkin;A. Placidi;E. Placidi;M. L. Planas;W. Plastino;C. Pluchar;R. Poggiani;E. Polini;D. T. Pong;S. Ponrathnam;E. Porter;R. Poulton;A. Poverman;J. Powell;M. Pracchia;T. Pradier;A. K. Prajapati;K. Prasai;R. Prasanna;G. Pratten;M. Principe;G. Prodi;L. Prokhorov;P. Prosposito;L. Prudenzi;A. Puecher;M. Punturo;F. Puosi;P. Puppo;M. Purrer;H. Qi;N. Quartey;V. Quetschke;P. J. Quinonez;R. Quitzow-James;F. Raab;G. Raaijmakers;H. Radkins;N. Radulesco;P. Raffai;S. X. Rail;S. Raja;C. Rajan;K. Ramirez;T. Ramirez;A. Ramos-Buades;J. Rana;P. Rapagnani;A. Ray;V. Raymond;N. Raza;M. Razzano;J. Read;L. A. Rees;T. Regimbau;L. Rei;S. Reid;S. Reid;D. Reitze;P. Relton;A. Renzini;P. Rettegno;B. Revenu;A. Reza;M. Rezac;F. Ricci;D. Richards;J. Richardson;L. Richardson;G. Riemenschneider;K. Riles;S. Rinaldi;K. Rink;N. Robertson;R. Robie;F. Robinet;A. Rocchi;S. Rodriguez;L. Rolland;J. Rollins;M. Romanelli;R. Romano;C. Romel;A. Romero;I. Romero-Shaw;J. Romie;S. Ronchini;L. Rosa;C. Rose;D. Rosi'nska;M. Ross;S. Rowan;S. Rowlinson;S. Roy;S. Roy;S. Roy;D. Rozza;P. Ruggi;K. Ruiz-Rocha;K. Ryan;S. Sachdev;T. Sadecki;J. Sadiq;S. Saha;Y. Saito;K. Sakai;M. Sakellariadou;S. Sakon;O. Salafia;F. Salces-Carcoba;L. Salconi;M. Saleem;F. Salemi;A. Samajdar;E. Sanchez;J. H. Sánchez;L. Sanchez;N. Sanchis-Gual;J. Sanders;A. Sanuy;T. R. Saravanan;N. Sarin;B. Sassolas;H. Satari;O. Sauter;R. Savage;V. Savant;T. Sawada;H. Sawant;S. Sayah;D. Schaetzl;M. Scheel;J. Scheuer;M. Schiworski;P. Schmidt;S. Schmidt;R. Schnabel;M. Schneewind;R. Schofield;A. Schonbeck;B. Schulte;B. Schutz;E. Schwartz;J. Scott;S. Scott;M. Seglar-Arroyo;Y. Sekiguchi;D. Sellers;A. Sengupta;D. Sentenac;E. Seo;V. Sequino;A. Sergeev;Y. Setyawati;T. Shaffer;M. Shahriar;M. Shaikh;B. Shams;L. Shao;A. Sharma;P. Sharma;P. Shawhan;N. Shcheblanov;A. Sheela;Y. Shikano;M. Shikauchi;H. Shimizu;K. Shimode;H. Shinkai;T. Shishido;A. Shoda;D. Shoemaker;D. Shoemaker;S. Shyamsundar;M. Sieniawska;D. Sigg;L. Silenzi;L. Singer;D. Singh;M. Singh;N. Singh;A. Singha;A. Sintes;V. Sipala;V. Skliris;B. Slagmolen;T. Slaven-Blair;J. Smetana;J. R. Smith;L. Smith;R. Smith;J. Soldateschi;S. Somala;K. Somiya;I. Song;K. Soni;V. Sordini;F. Sorrentino;N. Sorrentino;R. Soulard;T. Souradeep;E. Sowell;V. Spagnuolo;A. Spencer;M. Spera;P. Spinicelli;A. Srivastava;V. Srivastava;K. Staats;C. Stachie;F. Stachurski;D. Steer;J. Steinlechner;S. Steinlechner;N. Stergioulas;D. Stops;M. Stover;K. Strain;L. Strang;G. Stratta;M. D. Strong;A. Strunk;R. Sturani;A. Stuver;M. Suchenek;S. Sudhagar;V. Sudhir;R. Sugimoto;H. Suh;A. G. Sullivan;T. Summerscales;L. Sun;S. Sunil;A. Sur;J. Suresh;P. Sutton;Takamasa Suzuki;Takanori Suzuki;Toshikazu Suzuki;B. Swinkels;M. J. Szczepa'nczyk;P. Szewczyk;M. Tacca;H. Tagoshi;S. Tait;H. Takahashi;R. Takahashi;S. Takano;H. Takeda;M. Takeda;C. Talbot;C. Talbot;K. Tanaka;Taiki Tanaka;Takahiro Tanaka;A. Tanasijczuk;S. Tanioka;D. Tanner;D. Tao;L. Tao;R. D. Tapia;E. Mart'in;C. Taranto;A. Taruya;J. Tasson;R. Tenorio;J. Terhune;L. Terkowski;M. Thirugnanasambandam;M. Thomas;P. Thomas;E. E. Thompson-E.;J. Thompson;S. R. Thondapu;K. Thorne;E. Thrane;S. Tiwari;S. Tiwari;V. Tiwari;A. Toivonen;A. Tolley;T. Tomaru;T. Tomura;M. Tonelli;Z. Tornasi;A. Torres-Forn'e;C. Torrie;I. T. E. Melo;D. Toyra;A. Trapananti;F. Travasso;G. Traylor;M. Trevor;M. Tringali;A. Tripathee;L. Troiano;A. Trovato;L. Trozzo;R. Trudeau;D. Tsai;K. W. Tsang;T. Tsang;J. Tsao;M. Tse;R. Tso;S. Tsuchida;L. Tsukada;D. Tsuna;T. Tsutsui;K. Turbang;M. Turconi;D. Tuyenbayev;A. Ubhi;N. Uchikata;T. Uchiyama;R. Udall;A. Ueda;T. Uehara;K. Ueno;G. Ueshima;C. Unnikrishnan;A. Urban;T. Ushiba;A. Utina;G. Vajente;A. Vajpeyi;G. Valdes;M. Valentini;V. Valsan;N. Bakel;M. Beuzekom;M. Dael;J. Brand;C. Broeck;D. Vander-Hyde;H. Haevermaet;J. V. Heijningen;M. Putten;N. Remortel;M. Vardaro;A. Vargas;V. Varma;M. Vas'uth;A. Vecchio;G. Vedovato;J. Veitch;P. Veitch;J. Venneberg;G. Venugopalan;D. Verkindt;P. Verma;Y. Verma;Sander M. Vermeulen;D. Veske;F. Vetrano;A. Vicer'e;S. Vidyant;A. Viets;A. Vijaykumar;V. Villa-Ortega;J. Vinet;A. Virtuoso;S. Vitale;H. Vocca;E. V. Reis;J. Wrangel;C. Vorvick;S. Vyatchanin;L. Wade;M. Wade;K. Wagner;R. Walet;M. Walker;G. Wallace;L. Wallace;J. Wang;J. Wang;W. H. Wang;R. Ward;J. Warner;M. Was;T. Washimi;N. Y. Washington;J. Watchi;B. Weaver;C. Weaving;S. Webster;M. Weinert;A. Weinstein;R. Weiss;C. Weller;R. Weller;F. Wellmann;L. Wen;P. Wessels;K. Wette;J. Whelan;D. White;B. Whiting;C. Whittle;D. Wilken;D. Williams;M. Williams;A. Williamson;J. Willis;B. Willke;D. Wilson;C. Wipf;T. Włodarczyk;G. Woan;J. Woehler;J. Wofford;D. Wong;I. C. Wong;M. Wright;C. Wu;D. Wu;H. Wu;D. Wysocki;L. Xiao;T. Yamada;H. Yamamoto;K. Yamamoto;T. Yamamoto;K. Yamashita;R. Yamazaki;F. Yang;K. Z. Yang;L. Yang;Y. Yang;Y. Yang;Yang Yang-Yang;M. Yap;D. Yeeles;S. Yeh;A. Yelikar;M. Ying;J. Yokoyama;T. Yokozawa;J. Yoo;T. Yoshioka;Hang Yu;Haocun Yu;H. Yuzurihara;A. Zadro.zny;M. Zanolin;S. Zeidler;T. Zelenova;J. Zendri;M. Zevin;M. Zhan;H. Zhang;J. Zhang;L. Zhang;R. Zhang;T. Zhang;Y. Zhang;C. Zhao;G. Zhao;Y. Zhao;Yue Zhao;R. Zhou;Z. Zhou;X. Zhu;Z. Zhu;M. Zucker;J. Zweizig

Observation of Gravitational Waves from Two Neutron Star-Black Hole Coalescences

• DOI: 10.3847/2041-8213/ac082e
• 发表时间: 2021-07-01
• 期刊: ASTROPHYSICAL JOURNAL LETTERS
• 影响因子: 7.9
• 作者: Abbott, R.;Abbott, T. D.;Zweizig, J.
• 通讯作者: Zweizig, J.

Avoiding a Cluster Catastrophe: Retention Efficiency and the Binary Black Hole Mass Spectrum

避免集群灾难：保留效率和二元黑洞质谱

• DOI: 10.3847/2041-8213/ac853d
• 发表时间: 2022
• 期刊: The Astrophysical Journal Letters
• 作者: Zevin, Michael;Holz, Daniel E.
• 通讯作者: Holz, Daniel E.