Exploring the sensitivity of next generation gravitational wavedetectors Article Swipe
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Physics
Gravitational wave
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Sensitivity (control systems)
Gravitational-wave observatory
Einstein Telescope
Universe
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Binary number
Astronomy
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Electronic engineering
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B. P. Abbott
,
R. Abbott
,
T. D. Abbott
,
M. R. Abernathy
,
K. Ackley
,
C. Adams
,
P. Addesso
,
R. X. Adhikari
,
V. B. Adya
,
C. Affeldt
,
N. Aggarwal
,
O. D. Aguiar
,
A. Ain
,
P. Ajith
,
B. Allen
,
P. A. Altin
,
S. B. Anderson
,
W. G. Anderson
,
K. Arai
,
M. C. Araya
,
C. C. Arceneaux
,
J. S. Areeda
,
K. G. Arun
,
G. Ashton
,
M. Ast
,
S. M. Aston
,
P. Aufmuth
,
C. Aulbert
,
S. Babak
,
P. T. Baker
,
S. Ballmer
,
J. C. Barayoga
,
S. E. Barclay
,
B. C. Barish
,
D. Barker
,
B. Barr
,
L. Barsotti
,
J. Bartlett
,
I. Bartos
,
R. Bassiri
,
J. C. Batch
,
C. Baune
,
A. S. Bell
,
B. K. Berger
,
G. Bergmann
,
C. P. L. Berry
,
J. Betzwieser
,
S. Bhagwat
,
R. Bhandare
,
I. A. Bilenko
,
G. Billingsley
,
J. Birch
,
R. Birney
,
Sébastien Biscans
,
A. Bisht
,
C. Biwer
,
J. K. Blackburn
,
C. D. Blair
,
D. G. Blair
,
R. M. Blair
,
O. Bock
,
C. Bogan
,
A. Bohé
,
C. Bond
,
R. Bork
,
S. Bose
,
P. R. Brady
,
V. B. Braginsky
,
J. E. Brau
,
M. Brinkmann
,
P. Brockill
,
J. E. Broida
,
A. F. Brooks
,
D. Brown
,
D. Brown
,
N. M. Brown
,
S. Brunett
,
C. C. Buchanan
,
A. Buikema
,
A. Buonanno
,
Robert L. Byer
,
M. Cabero
,
L. Cadonati
,
C. Cahillane
,
J. Calderón Bustillo
,
T. A. Callister
,
J. B. Camp
,
K. C. Cannon
,
J. Cao
,
C. D. Capano
,
S. Caride
,
S. Caudill
,
M. Cavaglià
,
C. Cepeda
,
S. J. Chamberlin
,
M. Chan
,
S. Chao
,
P. Charlton
,
B. D. Cheeseboro
,
Yu‐Hung Chen
·
YOU?
·
· 2017
· Open Access
·
· DOI: https://doi.org/10.1088/1361-6382/aa51f4
· OA: W2502015268
YOU?
·
· 2017
· Open Access
·
· DOI: https://doi.org/10.1088/1361-6382/aa51f4
· OA: W2502015268
The second-generation of gravitational-wave detectors are just starting operation, and have already yielding their first detections. Research is now concentrated on how to maximize the scientific potential of gravitational-wave astronomy. To support this effort, we present here design targets for a new generation of detectors, which will be capable of observing compact binary sources with high signal-to-noise ratio throughout the Universe.
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