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Antimicrobials: a global alliance for optimizing their rational use in intra-abdominal infections (AGORA)

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Publication venue: 'Springer Science and Business Media LLC'
Publication date: 01/01/2016
Field of study

Intra-abdominal infections (IAI) are an important cause of morbidity and are frequently associated with poor prognosis, particularly in high-risk patients. The cornerstones in the management of complicated IAIs are timely effective source control with appropriate antimicrobial therapy. Empiric antimicrobial therapy is important in the management of intra-abdominal infections and must be broad enough to cover all likely organisms because inappropriate initial antimicrobial therapy is associated with poor patient outcomes and the development of bacterial resistance. The overuse of antimicrobials is widely accepted as a major driver of some emerging infections (such as C. difficile), the selection of resistant pathogens in individual patients, and for the continued development of antimicrobial resistance globally. The growing emergence of multi-drug resistant organisms and the limited development of new agents available to counteract them have caused an impending crisis with alarming implications, especially with regards to Gram-negative bacteria. An international task force from 79 different countries has joined this project by sharing a document on the rational use of antimicrobials for patients with IAIs. The project has been termed AGORA (Antimicrobials: A Global Alliance for Optimizing their Rational Use in Intra-Abdominal Infections). The authors hope that AGORA, involving many of the world's leading experts, can actively raise awareness in health workers and can improve prescribing behavior in treating IAIs

Archivio Istituzionale della Ricerca - Università degli Studi di Pavia

Archivio istituzionale della ricerca - Università dell'Insubria

Ghent University Academic Bibliography

Archivio della Ricerca - Università di Pisa

Spiral - Imperial College Digital Repository

Repositorio da Producao Cientifica e Intelectual da Unicamp

Study of B Meson Production in p plus Pb Collisions at root s(NN)=5.02 TeV Using Exclusive Hadronic Decays

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Publication venue
Publication date: 01/01/2015
Field of study

Peer reviewe

Full-text Institutional Repository of the Ruđer Bošković Institute

Publikationsserver der RWTH Aachen University

Digital.CSIC

arXiv.org e-Print Archive

Çukurova University Institutional Repository

DIAL UCLouvain

OpenMETU (Middle East Technical University)

Biblos-e Archivo

Southampton (e-Prints Soton)

eResearch@Ozyegin

Florence Research

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Properties of the Binary Neutron Star Merger GW170817

Author: A
A
A
A. S
Abbott B. P
Abbott R
Abbott T. D
Abhirup and Ghosh
Acernese F
Ackley K
Adams C
Adams T
Addesso P
Adhikari R. X
Adya V. B
Affeldt C
Agarwal B
Agathos M
Agatsuma K
Aggarwal N
Aguiar O. D
Aiello L
Ain A
Ajith P
Allen B
Allen G
Allocca A
Aloy M. A
Altin P. A
Amato A
Ananyeva A
Anderson S. B
Anderson W. G
Angelova
Antier S
Appert S
Arai K
Araya M. C
Archisman and Ghosh
Areeda J. S
Arene M
Arnaud N
Arun K. G
Arunava and Mukherjee
Ascenzi S
Ashton G
Ast M
Aston S. M
Astone P
Atallah
Aubin F
Aufmuth P
Aulbert C
AultONeal K
Austin C
Avila-Alvarez A
B
B
B
Babak S
Bacon P
Badaracco F
Bader M. K. M
Bae S
Baker P. T
Baldaccini F
Ballardin G
Ballmer S. W
Banagiri S
Barayoga J. C
Barclay S. E
Barish B. C
Barker D
Barkett K
Barnum S
Barone F
Barr B
Barsotti L
Barsuglia M
Barta D
Bartlett J
Bartos
Basti A
Batch J. C
Bawaj M
Bayley J. C
Bazzan M
Becsy B
Beer C
Bejger M
Belahcene
Beniwal D
Bensch M
Berger B. K
Bergmann G
Bernuzzi S
Bero J. J
Berry C. P. L
Bersanetti D
Bertolini A
Betzwieser J
Bhandare R
Bilenko I. A
Bilgili S. A
Billingsley G
Billman C. R
Birch J
Birney R
Birnholtz O
Biscans S
Biscoveanu S
Bisht A
Bitossi M
Bizouard M. A
Blackburn J. K
Blackman J
Blair C. D
Blair D. G
Blair R. M
Bloemen S
Bock O
Bode N
Boer M
Boetzel Y
Bogaert G
Bohe A
Bondu F
Bonilla E
Bonnand R
Booker P
Boom B. A
Booth C. D
Bork R
Boschi
Bossie K
Bossilkov
Bouffanais Y
Bozzi A
Bradaschia C
Brady P. R
Bramley A
Branchesi M
Brau J. E
Briant T
Brighenti F
Brillet A
Brinkmann M
Brisson
Brooks A. F
Brown D. D
Brunett S
Buchanan C. C
Buikema A
Bulik T
Bulten H. J
Buonanno A
Buskulic D
Bustillo
Buy C
Byer R. L
C
C
C
C
C-J and Haughian
Cabero M
Cadonati L
Cagnoli G
Cahillane C
Calloni E
Camp J. B
Canepa M
Canizares P
Cannon K. C
Cao H
Cao J
Capano C. D
Capocasa E
Carbognani F
Caride S
Carney M. F
Carullo G
Castro
Caudill S
Cavaglia M
Cavalier F
Cavalieri R
Cella G
Cepeda C. B
Cerda-Duran P
Cerretani G
Cesarini E
Chaibi O
Chamberlin S. J
Chan M
Chao S
Charlton P
Chase E
Chassande-Mottin E
Chatterjee D
Chatziioannou K
Cheeseboro B. D
Chen H. Y
Chen X
Chen Y
Cheng
Chincarini A
Chiummo A
Chmiel T
Cho H. S
Cho M
Chow J. H
Christensen N
Chu Q
Chua A. J. K
Chua S
Chung K. W
Chung S
Chunglee and Kim
Ciani G
Ciobanu A. A
Ciolfi R
Cipriano F
Cirelli C. E
Cirone A
Clara F
Clark J. A
Clearwater P
Cleva F
Cocchieri C
Coccia E
Cohadon
Colla A
Collette C. G
Collins C
Cominsky L. R
Constancio M
Conti L
Cooper S. J
Corban P
Corbitt T. R
Cordero-Carrion
Cornish N
Corsi A
Cortese S
Costa C. A
Cotesta R
Coughlin M. W
Coughlin S. B
Coulon
Couvares P
Covas P. B
Cowan E. E
Coward D. M
Cowart M. J
Coyne D. C
Coyne R
Creighton J. D. E
Creighton T. D
Cripe J
Crowder S. G
Cullen T. J
Cumming A
Cunningham L
Cuoco E
D
D
D
D
D
D
D'Antonio S
D. B
Da Silva Costa C. F
Dal Canton T
Dalya G
Danilishin S. L
Danzmann K
Dasgupta A
Dattilo
Davis D
Daw E. J
Day B
De Laurentis M
De Pietri R
De Rossi C
de Varona O
DeBra D
Deenadayalan M
Degallaix J
Del Pozzo W
Deleglise S
Demos N
Denker T
Dent T
Derby J
Dergachev
DeSalvo R
Dhurandhar S
Di Fiore L
Di Giovanni M
Di Girolamo T
Di Lieto A
Di Pace S
Di Palma
Diaz
Diaz M. C
Dietrich T
Ding B
Dmitriev A
Doctor Z
Dolique
Dooley K. L
Doravari S
Dorrington
Drago M
Dreissigacker C
Driggers J. C
Du Z
Dudi R
Dupej P
Dwyer S. E
E. A
E. C
E. J
Easter P. J
Edo T. B
Edwards M. C
Effler A
Eggenstein
Eichhol J
Eikenberry S. S
Eisenmann M
Eisenstein R. A
Essick R. C
Estelles H
Estevez D
Etienne Z. B
Etzel T
Evans M
Evans T. M
F
F
F
Fafone
Fairhurst S
Fan X
Farinon S
Farr B
Farr W. M
Fauchon-Jones E. J
Favata M
Fays M
Fee C
Fehrmann H
Feicht J
Fejer M. M
Feng F
Fernandez-Galiana A
Ferrante
Ferrini F
Fidecaro F
Fiori
Fishbach M
Fisher R. P
Fishner J. M
Fitz-Axen M
Flaminio R
Fletcher M
Fong H
Font J. A
Forsyth P. W. F
Forsyth S. S
Fournier
Frasconi F
Frei Z
Freise A
Frey
Frey R
Frolov V. V
Fulda P
Fyffe M
G
G
G. L
Gabbard H. A
Gadre B. U
Gaebel S. M
Gair J. R
Gammaitoni L
Ganija M. R
Gaonkar S. G
Garcia A
Garcia-Quiros C
Garufi F
Gateley B
Gaudio S
Gaur G
Gayathri
Genin E
Gennai A
George D
George J
Gergely L
Germain
Ghosh
Giacomazzo B
Giaime J. A
Giardina K. D
Giazotto A
Gill K
Giordano G
Glover L
Goetz E
Goetz R
Goncharov B
Gonzalez G
Gorodetsky M. L
Gossan S. E
Gosselin M
Gouaty R
Grado A
Graef C
Granata M
Grant A
Gras S
Gray C
Greco G
Green A. C
Green R
Gretarsson E. M
Groot P
Grote H
Grunewald S
Gruning P
Guidi G. M
Gulati H. K
Guo X
Gupta A
Gupta M. K
Gushwa K. E
Gustafson E. K
Gustafson R
H
H-B and Ehrens
H-P and Chia
H. Y
Halim O
Hall B. R
Hall E. D
Hamilton E. Z
Hamilton H. F
Hammond G
Haney M
Hang and Yu
Hanke M. M
Hanks J
Hanna C
Hannam M. D
Hannuksela O. A
Hanson J
Haocun and Yvert
Hardwick T
Harms J
Harry G. M
Harry I. W
Hart M. J
Haster
Healy J
Heidmann A
Heintze M. C
Heitmann H
Hello P
Hemming G
Hendry M
Heng I. S
Hennig J
Heptonstall A. W
Hernandez
Hernandez F. J
Heurs M
Hild S
Hinderer T
Hoak D
Hochheim S
Hofman D
Holland N. A
Holtz K
Holz D. E
Hopkins P
Horst C
Hough J
Houston E. A
Howard and Pan
Howell E. J
Hreibi A
Huang-Wei and Pang
Huerta E. A
Huet D
Hughey B
Hulko M
Husa S
Huttner S. H
Huynh-Dinh T
I
I
I and Alvarez
I and Bassiri
I and Bell
I and Corley
I and Davier
I and Di Renzo
I and Ferreira
I and Fiorucci
I and Khan
I and Kozak
I and Man
I and Naticchioni
I. Magana and Magana-Sandoval
Iess A
Indik N
Ingram C
Inta R
Intini G
Isa H. N
Isac
Iyer B. R
Izumi K
J
J
J-D and Frasca
J-M and Isi
J-P and Countryman
J-P and Zevin
J-Y and Vitale
J. C
J. Caldron and Callister
J. Casanueva and Casentini
J. M. Gonzalez and Gopakumar
J. R
Jacqmin T
Jani K
Jaranowski P
Javed and Rapagnani
Johnson D. S
Johnson W. W
Jones
Jones R
Jonker R. J. G
Ju L
Junker J
K
K
K. R
Kalaghatgi
Kalogera
Kandhasamy S
Kang G
Kanner J. B
Kapadia S. J
Karki S
Karvinen K. S
Kasprzack M
Kastaun W
Katolik M
Katsanevas S
Katsavounidis E
Katzman W
Kaufer S
Kawabe K
Keerthana
Kefelian F
Keitel D
Kemball A. J
Kennedy R
Key J. S
Khalili F. Y
Khamesra B
Khan
Khan H
Khan Z
Khazanov E. A
Kijbunchoo N
Kim
Kim
Kim K
Kim W
Kim W. S
King P. J
Kinley-Hanlon M
Kirchhoff R
Kissel J. S
Kleybolte L
Klimenko S
Knowles T. D
Koch P
Koehlenbeck S. M
Koley S
Kondrashov
Korobko M
Korth W. Z
Kowalska
Kraemer C
Kringel
Krolak A
Kuehn G
Kumar P
Kumar R
Kumar S
Kuo L
Kutynia A
Kwang S
L
L-W and Weinert
L. Magana and Magee
Lackey B. D
Lai K. H
Landry M
Landry P
Lang R. N
Lange J
Lantz B
Lanza R. K
Lartaux-Vollard A
Lasky P. D
Laxen M
Lazzarini A
Lazzaro C
Leaci P
Leavey S
Lee C. H
Lee H. K
Lee H. M
Lee H. W
Lee K
Lehmann J
Lenon A
Leonardi M
Leroy N
Letendre N
Levin Y
Li J
Li T. G. F
Li X
LIGO Sci Collaboration and Virgo Collaboration
Linker S. D
Littenberg T. B
Liu J
Liu X
Lo R. K. L
Lockerbie N. A
London L. T
Longo A
Lorenzini M
Loriette
Losurdo G
Lough J. D
Lousto C. O
Lovelace G
Lueck H
Lumaca D
Lundgren A. P
Lynch R
M
M
M
M
M
M
M
M. Dovale and Downes
Ma Y
Macas R
Macfoy S
Machenschalk B
MacInnis M
Macleod D. M
Majorana E
Maksimovic
Mandic
Manske M
Mantovani M
Marchesoni F
Marion F
Marka S
Marka Z
Markakis C
Markosyan A. S
Markowitz A
Maros E
Marquina A
Martelli F
Martellini L
Martin I. W
Martin R. M
Martynov
Mason K
Massera E
Masserot A
Massinger T. J
Masso-Reid M
Mastrogiovanni S
Matas A
Matichard F
Matone L
Mavalvala N
Mazumder N
McCann J. J
McCarthy R
McClelland D. E
McCormick S
McCuller L
McGuire S. C
McIver J
McManus D. J
McRae T
McWilliams S. T
Meacher D
Meadors G. D
Mehmet M
Meidam J
Mejuto-Villa E
Melatos A
Mendell G
Mendoza-Gandara D
Mercer R. A
Mereni L
Merilh E. L
Merzougui M
Meshkov S
Messenger C
Messick C
Metzdorff R
Meyers P. M
Miao H
Michel C
Middleton H
Mikhailov E. E
Milano L
Miller A
Miller A. L
Miller B. B
Miller J
Millhouse M
Mills J
Milovich-Goff M. C
Minazzoli O
Minenkov Y
Ming J
Mishra C
Mitra S
Mitrofanov V. P
Mitselmakher G
Mittleman R
Moffa D
Mogushi K
Mohan M
Mohapatra S. R. P
Montani M
Moore C. J
Moraru D
Moreno G
Morisaki S
Mours B
Mow-Lowry C. M
Mueller G
Muir A. W
Mukherjee
Mukherjee S
Mukund N
Mullavey A
Munch J
Muniz E. A
Muratore M
Murray P. G
N
N
Nagar A
Napier K
Nardecchia
Nayak R. K
Neilson J
Nelemans G
Nelson T. J. N
Nery M
Neunzert A
Nevin L
Newport J. M
Ng K. Y
Ng S
Nguyen P
Nguyen T. T
Nichols D
Nielsen A. B
Nissanke S
Nitz A
Nocera F
Nolting D
North C
Nuttall L. K
O'Brien B. D
O'Dea G. D
O'Reilly B
O'Shaughnessy R
Obergaulinger M
Oberling J
Ogin G. H
Oh J. J
Oh S. H
Ohme F
Ohta H
Okada M. A
Oliver M
Oppermann P
Oram Richard J
Ormiston R
Ortega L. F
Ossokine S
Ottaway D. J
Overmier H
Owen B. J
P
P
P
P
P-F and Cohen
Pace A. E
Pagano G
Page J
Page M. A
Pai A
Pai S. A
Pal-Singh A
Palamos J. R
Palashov O
Palomba C
Pan
Pang P. T. H
Pankow C
Pannarale F
Pant B. C
Paoletti F
Paoli A
Papa M. A
Parida A
Parker W
Pascucci D
Pasqualetti A
Passaquieti R
Passuello D
Patil M
Patricelli B
Pearlstone B. L
Pedersen C
Pedraza M
Pedurand R
Pekowsky L
Pele A
Penn S
Perez C. J
Perreca A
Perri L. M
Pfeiffer H. P
Phelps M
Phukon K. S
Piccinni O. J
Pichot M
Piergiovanni F
Pierro
Pinard L
Pinto I. M
Pirello M
Pitkin M
Poggiani R
Popolizio P
Porter E. K
Possenti L
Post A
Powell J
Prasad J
Pratt J. W. W
Pratten G
Predoi
Principe M
Privitera S
Prodi G. A
Prokhorov L. G
Prrer M
Puncken O
Punturo M
Puppo P
Qi H
Quetschke
Quitzow-James R
R
R
R. M
Raab F. J
Rabeling D. S
Radkins H
Raffai P
Raja S
Rajan C
Rajbhandari B
Rakhmanov M
Ramirez K. E
Ramos-Buades A
Rana
Raymond
Read J
Regimbau T
Rei L
Reid S
Reitze D. H
Ren W
Ricci F
Ricker P. M
Riemenschneider G
Riles K
Rizzo M
Robertson N. A
Robie R
Robinet F
Robson T
Rocchi A
Rolland L
Rollins J. G
Roma V. J
Romano R
Romel C. L
Romie J. H
Rosinska D
Ross M. P
Rowan S
Ruediger A
Ruggi P
Rutins G
Ryan K
S
S
S
S
S
S
S
S
S. T
Sachdev S
Sadecki T
Sakellariadou M
Salconi L
Saleem M
Salemi F
Samajdar A
Sammut L
Sampson L. M
Sanchez E. J
Sanchez L. E
Sanchis-Gual N
Sandberg
Sarin N
Sassolas B
Sathyaprakash B. S
Saulson P. R
Sauter O
Savage R. L
Sawadsky A
Schale P
Scheel M
Scheuer J
Schmidt P
Schnabel R
Schoenbeck A
Schofield R. M. S
Schreiber E
Schuette D
Schulte B. W
Schutz B. F
Schwalbe S. G
Scott J
Scott S. M
Seidel E
Sellers D
Sengupta A. S
Sentenac D
Sequino
Setyawati Y
Shaddock D. A
Shaffer T. J
Shah A. A
Shahriar M. S
Shaner M. B
Shao L
Shapiro B
Shawhan P
Shen H
Shoemaker D. H
Shoemaker D. M
Siellez K
Siemens X
Sieniawska M
Sigg D
Silva A. D
Singer L. P
Singh A
Singhal A
Sintes A. M
Slagmolen B. J. J
Slaven-Blair T. J
Smith B
Smith J. R
Smith R. J. E
Somala S
Son E. J
Sorazu B
Sorrentino F
Souradeep T
Spencer A. P
Srivastava A. K
Staats K
Steinke M
Steinlechner J
Steinlechner S
Steinmeyer D
Steltner B
Stevenson S. P
Stocks D
Stone R
Stops D. J
Strain K. A
Stratta G
Strigin S. E
Strunk A
Sturani R
Stuver A. L
Summerscales T. Z
Sun L
Sunil S
Suresh J
Sutton P. J
Swinkels B. L
Szczepanczyk M. J
T
T. A
T. P
Tacca M
Tait S. C
Talbot C
Talukder D
Tanner D. B
Tapai M
Taracchini A
Tasson J. D
Taylor J. A
Taylor R
Tewari
Theeg T
Thies F
Thomas E. G
Thomas M
Thomas P
Thorne K. A
Thrane E
Tiwari
Tiwari S
Toeyrae D
Toland K
Tonelli M
Tornasi Z
Torres-Forne A
Torrie
Travasso F
Traylor G
Trinastic J
Tringali M. C
Trozzo L
Tsang K. W
Tse M
Tso R
Tsukada L
Tsuna D
Tuyenbayev D
Ueno K
Ugolini D
Urban A. L
Usman S. A
V
V
V
V
V
V
V
V
V and Bose
V and Bosveld
V and Brockill
V and Dave
V and De Rosa
V and Donovan
V and Fair
V and Fritschel
V and Gemme
V and Ghonge
V and Kamai
V and Kontos
V and Krishnan
V and Lormand
V and Mangano
V and Mansell
V and Pillant
V and Prestegard
V and Quintero
V and Razzano
V and Sanders
V and Sergeev
V and Tokmakov
Vahlbruch H
Vajente G
Valdes G
van Bakel N
van Beuzekom M
van den Brand J. F. J
van den Broeck C
van der Schaaf L
van Heijningen
van Veggel A. A
vander-Hyde D. C
Vardaro M
Varma V
Vass S
Vasuth M
Vecchio A
Vedovato G
Veitch J
Veitch P. J
Venkateswara K
Venugopalan G
Verkindt D
Vetrano F
Vicere A
Viets A. D
Vinciguerra S
Vine D. J
Vinet
Vo T
Vocca H
Vorvick C
Vyatchanin S. P
Wade A. R
Wade L. E
Wade M
Walet R
Walker M
Wallace L
Walsh S
Wang G
Wang H
Wang J. Z
Wang W. H
Wang Y. F
Ward R. L
Warner J
Was M
Watchi J
Weaver B
Wei
Weinstein A. J
Weiss R
Wellmann F
Wen L
Wessel E. K
Wessels P
Westerweck J
Wette K
Whelan J. T
Whiting B. F
Whittle C
Wilken D
Williams D
Williams R. D
Williamson A. R
Willis J. L
Willke B
Wimmer M. H
Winkler W
Wipf C. C
Wittel H
Woan G
Woehler J
Wofford J. K
Wong W. K
Worden J
Wright J. L
Wu D. S
Wysocki D. M
Xiao S
Y-H and Zhao
Y-M and King
Yam W
Yamamoto H
Yancey C. C
Yang L
Yap M. J
Yazback M
Yu
Zadrozny A
Zanolin M
Zelenova T
Zendri
Zertuche
Zhang
Zhang J
Zhang L
Zhang M
Zhang T
Zhou M
Zhou Z
Zhu S. J
Zhu X. J
Zimmerman A. B
Zlochower Y
Zucker M. E
Zweizig J
Publication venue: 'American Physical Society (APS)'
Publication date: 01/01/2019
Field of study

On August 17, 2017, the Advanced LIGO and Advanced Virgo gravitational-wave detectors observed a low-mass compact binary inspiral. The initial sky localization of the source of the gravitational-wave signal, GW170817, allowed electromagnetic observatories to identify NGC 4993 as the host galaxy. In this work, we improve initial estimates of the binary's properties, including component masses, spins, and tidal parameters, using the known source location, improved modeling, and recalibrated Virgo data. We extend the range of gravitational-wave frequencies considered down to 23 Hz, compared to 30 Hz in the initial analysis. We also compare results inferred using several signal models, which are more accurate and incorporate additional physical effects as compared to the initial analysis. We improve the localization of the gravitational-wave source to a 90% credible region of 16 deg2. We find tighter constraints on the masses, spins, and tidal parameters, and continue to find no evidence for nonzero component spins. The component masses are inferred to lie between 1.00 and 1.89 M⊙ when allowing for large component spins, and to lie between 1.16 and 1.60 M⊙ (with a total mass 2.73−0.01+0.04 M⊙) when the spins are restricted to be within the range observed in Galactic binary neutron stars. Using a precessing model and allowing for large component spins, we constrain the dimensionless spins of the components to be less than 0.50 for the primary and 0.61 for the secondary. Under minimal assumptions about the nature of the compact objects, our constraints for the tidal deformability parameter Λ are (0,630) when we allow for large component spins, and 300−230+420 (using a 90% highest posterior density interval) when restricting the magnitude of the component spins, ruling out several equation-of-state models at the 90% credible level. Finally, with LIGO and GEO600 data, we use a Bayesian analysis to place upper limits on the amplitude and spectral energy density of a possible postmerger signal

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Vinciguerra S
Vine D. J
Vinet
Vo T
Vocca H
Vorvick C
Vyatchanin S. P
Wade A. R
Wade L. E
Wade M
Walet R
Walker M
Wallace L
Walsh S
Wang H
Wang J. Z
Wang S
Wang W. H
Wang Y. F
Ward R. L
Warden Z. A
Warner J
Was M
Watchi J
Weaver B
Wei
Weinstein A. J
Weiss R
Wellmann F
Wen L
Wessel E. K
Wessels P
Westhouse J. W
Wette K
Whelan J. T
Whiting B. F
Whittle C
Wilken D. M
Williams D
Williamson A. R
Willis J. L
Willke B
Winkler W
Wipf C. C
Wittel H
Woan G
Woehler J
Wofford J. K
Wright J. L
Wu D. S
Wysocki D. M
Xiao S
Xu R
Y-M and Kimball
Yamamoto H
Yancey C. C
Yang L
Yang Y
Yang Z
Yap M. J
Yazback M
Yeeles D. W
Yu
Zadrozny A
Zadrozny A. K
Zanolin M
Zelenova T
Zendri
Zhang J
Zhang L
Zhang T
Zhao C
Zhao G
Zhou M
Zhou Z
Zhu X. J
Zucker M. E
Zweizig J
Publication venue: 'American Astronomical Society'
Publication date: 01/01/2019
Field of study

When formed through dynamical interactions, stellar-mass binary black holes (BBHs) may retain eccentric orbits (e > 0.1 at 10 Hz) detectable by ground-based gravitational-wave detectors. Eccentricity can therefore be used to differentiate dynamically formed binaries from isolated BBH mergers. Current template-based gravitational-wave searches do not use waveform models associated with eccentric orbits, rendering the search less efficient for eccentric binary systems. Here we present the results of a search for BBH mergers that inspiral in eccentric orbits using data from the first and second observing runs (O1 and O2) of Advanced LIGO and Advanced Virgo. We carried out the search with the coherent WaveBurst algorithm, which uses minimal assumptions on the signal morphology and does not rely on binary waveform templates. We show that it is sensitive to binary mergers with a detection range that is weakly dependent on eccentricity for all bound systems. Our search did not identify any new binary merger candidates. We interpret these results in light of eccentric binary formation models. We rule out formation channels with rates greater than about 100 Gpc−3 yr−1 for e > 0.1, assuming a black hole mass spectrum with a power-law index less than about 2

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