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Exploring the sensitivity of next generation gravitational wavedetectors
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, 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, 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, C. Cheng, H. S. Cho, M. Cho, J. H. Chow, N. Christensen, Q. Chu, S. Chung, G. Ciani, F. Clara, J. A. Clark, Christophe Collette, L. Cominsky, M. Constancio, D. Cook, T. R. Corbitt, Neil J. Cornish, A. Corsi, C. A. Costa, M. W. Coughlin, S. B. Coughlin, S. T. Countryman, P. Couvares, E. E. Cowan, D. M. Coward, M. J. Cowart, D. C. Coyne, R. Coyne, K. Craig, J. D. E. Creighton, J. Cripe, S. G. Crowder, A. Cumming, L. Cunningham, T. Dal Canton, S. L. Danilishin, K. Danzmann, N. S. Darman, Anirban Dasgupta, C. F. Da Silva Costa, I. Dave, G. S. Davies, E. J. Daw, D. DeBra, W. Del Pozzo, T. Denker, T. Dent, V. Dergachev, R. T. DeRosa, R. DeSalvo, R. C. Devine, S. Dhurandhar, M. C. Díaz, I. Di Palma, F. Donovan, K. L. Dooley, S. Doravari, R. Douglas, T. P. Downes, M. Drago, R. W. P. Drever, J. C. Driggers, S. E. Dwyer, T. B. Edo, M. C. Edwards, A. Effler, H-B Eggenstein, P. Ehrens, J. Eichholz, S. S. Eikenberry, W. Engels, R. C. Essick, T. Etzel, M. Evans, T. Evans, R. Everett, M. Factourovich, H. Fair, S. Fairhurst, X. Fan, Q. Fang, B. Farr, Will M. Farr, M. Favata, M. Fays, H. Fehrmann, M. M. Fejer, E. Fenyvesi, E. C. Ferreira, R. P. Fisher, M. Fletcher, Z. Frei, A. Freise, R. Frey, P. Fritschel, V. V. Frolov, P. Fulda, M. Fyffe, H. A. Gabbard, J. R. Gair, S. G. Gaonkar, G. Gaur, N. Gehrels, Peng Geng, J. George, L. Gergely, Abhirup Ghosh, Archisman Ghosh, J. A. Giaime, K. D. Giardina, K. Gill, A. Glaefke, E. Goetz, L. Gondán, G. González, A. Gopakumar, Neil Gordon, M. L. Gorodetsky, S. E. Gossan, C. Graef, P. B. Graff, A. Grant, S. Gras, C. Gray, A. C. Green, H. Grote, S. Grünewald, X. Guo, A. Gupta, Manoj Gupta, K. E. Gushwa, E. K. Gustafson, R. Gustafson, J. J. Hacker, E. D. Hall, G. Hammond, M. Haney, M. M. Hanke, J. Hanks, C. Hanna, M. D. Hannam, J. Hanson, T. Hardwick, I. W. Harry, M. J. Hart, M. T. Hartman, K. Haughian, M. C. Heintze, M. Hendry, I. S. Heng, J. Hennig, J. Henry, A. W. Heptonstall, M. Heurs, S. Hild, D. Hoak, K. Holt, D. E. Holz, P. Hopkins, J. Hough, E. A. Houston, E. J. Howell, Yi-Ming Hu, S. Huang, E. A. Huerta, B. Hughey, S. Husa, S. H. Huttner, T. Huynh–Dinh, N. Indik, D. R. Ingram, R. Inta, H. N. Isa, M. Isi, T. Isogai, B. R. Iyer, K. Izumi, H. Jang, K. Jani, S. Jawahar, L. K. Jian, F. Jiménez‐Forteza, W. W. Johnson, D. I. Jones, R. Jones, L. Ju, K. Haris, C. V. Kalaghatgi, V. Kalogera, S. Kandhasamy, G. Kang, J. B. Kanner, S. J. Kapadia, S. Karki, K. S. Karvinen, M. Kasprzack, E. Katsavounidis, W. Katzman, S. Kaufer, T. Kaur, K. Kawabe, M. S. Kehl, D. Keitel, D. B. Kelley, W. Kells, R. Kennedy, J. S. Key, F. Y. Khalili, S. Khan, Z. Khan, Е. А. Хазанов, N. Kijbunchoo, Chi-Woong Kim, Chunglee Kim, Jinwoo Kim, K. Kim, Nakwoo Kim, W. Kim, S. J. Kimbrell, E. J. King, Peter King, J. S. Kissel, Bernd Klein, L. Kleybolte, S. Klimenko, S. M. Koehlenbeck, V. Kondrashov, A. Kontos, M. Korobko, W. Z. Korth, D. B. Kozak, V. Kringel, C. Krueger, A. Królak, P. Kumar, S. Kumar, L. Kuo, B. D. Lackey, M. Landry, J. Lange, B. Lantz, P. D. Lasky, M. Laxen, A. Lazzarini, S. Leavey, E. O. Lebigot, Chang‐Hwan Lee, H. K. Lee, Hyung Mok Lee, K. Lee, A. Lenon, J. R. Leong, Y. Levin, J. B. Lewis, T G F Li, A. Libson, T. B. Littenberg, N. A. Lockerbie, A. L. Lombardi, L. T. London, J. E. Lord, M. Lormand, J. D. Lough, H. Lück, A. P. Lundgren, Ryan S. Lynch, Y. Ma, B. Machenschalk, M. MacInnis, D. M. Macleod, F. Magaña‐Sandoval, L. Magaña Zertuche, R. M. Magee, V. Mandic, V. Mangano, G. L. Mansell, Szabolcs Márka, Z. Márka, A. S. Markosyan, E. Maros, I. W. Martin, Д. В. Мартынов, K. Mason, T. J. Massinger, M. Masso‐Reid, F. Matichard, L. Matone, N. Mavalvala, N. Mazumder, R. McCarthy, D. E. McClelland, S. McCormick, S. C. McGuire, G. McIntyre, J. McIver, D. J. McManus, T. McRae, S. T. McWilliams, D. Meacher, G. D. Meadors, A. Melatos, G. Mendell, R. A. Mercer, E. L. Merilh, S. Meshkov, C. Messenger, C. Messick, P. M. Meyers, H. Miao, H. Middleton, Е. Е. Михайлов, A. L. Miller, B. B. Miller, J. Miller, M. Millhouse, J. Ming, S. Mirshekari, C. Mishra, S. Mitra, O. Miyakawa, G. Mitselmakher, R. Mittleman, M. Mondin, B. C. Moore, C. J. Moore, D. Moraru, G. Moreno, S. R. Morriss, K. Mossavi, C. M. Mow–Lowry, G. Mueller, A. W. Muir, Arunava Mukherjee, D. Mukherjee, S. Mukherjee, N. Mukund, A. Mullavey, J. Münch, D. Murphy, P. G. Murray, A. Mytidis, R. K. Nayak, K. Nedkova, T. J. N. Nelson, A. Neunzert, G. Newton, T. Nguyen, A. B. Nielsen, A. Nitz, D. Nolting, M. E. N. Normandin, L. K. Nuttall, J. Oberling, E. Ochsner, J. O’Dell, E. Oelker, G. H. Ogin, J. J. Oh, S. H. Oh, F. Ohme, M. Oliver, P. Oppermann, Richard J. Oram, B. O’Reilly, R. O’Shaughnessy, D. J. Ottaway, H. Overmier, B. J. Owen, A. Pai, S. A. Pai, J. R. Palamos, O. Palashov, A. Pal‐Singh, H. Pan, C. Pankow, F. Pannarale, B. C. Pant, M. A. Papa, H. R. Paris, W. Parker, D. Pascucci, Z. Patrick, B. L. Pearlstone, M. Pedraza, L. Pekowsky, A. Pele, S. Penn, A. Perreca, L. M. Perri, M. Phelps, V. Pierro, I. M. Pinto, M. Pitkin, M. Poe, A. Post, J. Powell, J. Prasad, V. Predoi, T. Prestegard, Larry R. Price, M. Prijatelj, M. Principe, S. Privitera, L. Prokhorov, O. Puncken, M. Pürrer, H. Qi, J. Qin, S. Qiu, V. Quetschke, E. A. Quintero, R. Quitzow-James, F. J. Raab, D. S. Rabeling, H. Radkins, P. Raffai, S. Raja, C. Rajan, M. Rakhmanov, V. Raymond, J. Read, C. M. Reed, S. Reid, D. H. Reitze, H. Rew, S. D. Reyes, K. Riles, Maria L. Rizzo, N. A. Robertson, R. Robie, J. G. Rollins, V. J. Roma, G. Romanov, J. H. Romie, S. Rowan, A. Rüdiger, K. Ryan, S. Sachdev, T. Sadecki, L. Sadeghian, Mairi Sakellariadou, M. Saleem, F. Salemi, A. Samajdar, L. Sammut, E. J. Sanchez, V. Sandberg, B. Sandeen, J. R. Sanders, B. S. Sathyaprakash, P. R. Saulson, R. L. Savage, A. Sawadsky, P. Schale, R. Schilling, P. Schmidt, R. Schnabel, R. M. S. Schofield, A. Schönbeck, E. Schreiber, D. Schuette, B. F. Schutz, J. Scott, S. M. Scott, D. Sellers, A. S. Sengupta, A. Sergeev, D. A. Shaddock, T. Shaffer, M. S. Shahriar, M. Shaltev, B. Shapiro, P. Shawhan, A. Sheperd, D. H. Shoemaker, D. M. Shoemaker, K. Siellez, X. Siemens, D. Sigg, A. D. Silva, A. Singer, L. P. Singer, A. Singh, R. Singh, A. M. Sintes, B. J. J. Slagmolen, J. R. Smith, N. D. Smith, R. J. E. Smith, E. J. Son, B. Sorazu, T. Souradeep, A. K. Srivastava, A. Staley, M. Steinke, J. Steinlechner, S. Steinlechner, D. Steinmeyer, B. C. Stephens, R. Stone, K. A. Strain, N. A. Strauss, S. Strigin, R. Sturani, A. L. Stuver, T. Z. Summerscales, L. Sun, P. J. Sutton, M. J. Szczepańczyk, D. Talukder, D. B. Tanner, M. Tápai, S. P. Tarabrin, A. Taracchini, R. Taylor, T. Theeg, M. P. Thirugnanasambandam, E. G. Thomas, M. Thomas, P. Thomas, K. A. Thorne, E. Thrane, V. Tiwari, K. V. Tokmakov, K. 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Bibliographic record
VenueClassical and Quantum Gravity · 2017
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of Toronto
FundersCalifornia Institute of TechnologyMassachusetts Institute of TechnologyScience and Technology Facilities CouncilNational Science Foundation
KeywordsPhysicsGravitational waveDetectorSensitivity (control systems)Gravitational-wave observatoryEinstein TelescopeUniverseGravitational-wave astronomyBinary numberAstronomyNoise (video)AstrophysicsOpticsElectronic engineering
Abstract
Abstract 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.
Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.
How this classification was reachedexpand
Full frame machine prediction
Teacher imitationNot calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.
metaresearch head score (Codex)0.002
metaresearch head score (Gemma)0.002
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.003
Threshold uncertainty score0.012
Distilled classifier scores by category (both heads)
| Category | Codex | Gemma |
|---|---|---|
| Metaresearch | 0.002 | 0.002 |
| Meta-epidemiology (narrow) | 0.001 | 0.000 |
| Meta-epidemiology (broad) | 0.001 | 0.000 |
| Bibliometrics | 0.001 | 0.000 |
| Science and technology studies | 0.000 | 0.000 |
| Scholarly communication | 0.002 | 0.002 |
| Open science | 0.001 | 0.002 |
| Research integrity | 0.002 | 0.001 |
| Insufficient payload (model declined to judge) | 0.003 | 0.001 |
Machine scores (provisional)
The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.
Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.
Opus teacher head0.155
GPT teacher head0.347
Teacher spread0.192 · how far apart the two teachers sit on this one work
Validation status
score_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from itClassification
machine, unvalidatedMachine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.
The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
Domainnot available
GenreEmpirical
How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".
Quick stats
Citations1,213
Published2017
Admission routes1
Has abstractyes