Zobrazeno 1 - 10
of 20
pro vyhledávání: '"R. T. Stebbins"'
Publikováno v:
Classical and Quantum Gravity. 21:S653-S660
The performance of the LISA gravitational wave detector depends critically on limiting spurious accelerations of the fiducial masses. Consequently, the requirements on allowable acceleration levels must be carefully allocated based on estimates of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::674065edc05160e7ae3ca4d44bab2906
https://doi.org/10.1088/0264-9381/21/5/039
https://doi.org/10.1088/0264-9381/21/5/039
Publikováno v:
Classical and Quantum Gravity. 20:S193-S199
Currently there are two implementations for LISA phase measurement being investigated in the United States. In this paper, we present the current status of one of these implementations, the so-called zero-crossing approach or stopwatch method. This m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::133dda1e9b698cb43b23f9f584f21f19
https://doi.org/10.1088/0264-9381/20/10/322
https://doi.org/10.1088/0264-9381/20/10/322
Publikováno v:
Classical and Quantum Gravity. 18:4159-4164
We present an experiment designed to test a type of phase measurement system that could be used for LISA. The set-up consists of two parts: one is an optical signal generator to provide an optical signal similar to that expected for the interferometr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6f170fc2ec02bc8d89b31d3973e89eeb
https://doi.org/10.1088/0264-9381/18/19/326
https://doi.org/10.1088/0264-9381/18/19/326
Publikováno v:
Review of Scientific Instruments. 69:2531-2538
The major obstacle to the detection of low-frequency gravitational waves with an earth-based interferometer is seismic noise. The current design of the initial Laser Interferometer Gravitational-Wave Observatory (LIGO) receiver, now under constructio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::50e3edda9486efe769d997b97482750c
https://doi.org/10.1063/1.1148954
https://doi.org/10.1063/1.1148954
Autor:
J. E. Mason, Peter L. Bender, R. T. Stebbins, Peter G. Nelson, D. B. Newell, S. J. Richman, James E. Faller
Publikováno v:
Review of Scientific Instruments. 68:3211-3219
To extend the operating frequency band of earth-based interferometric gravitational wave (GW) detectors down to 1 Hz, an unconventional system is required that provides approximately a factor of one million vibration isolation for the horizontal and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::26578cefe0f6f64bbed5872ab72763e1
https://doi.org/10.1063/1.1148269
https://doi.org/10.1063/1.1148269
Publikováno v:
Classical and Quantum Gravity. 14:1499-1505
Gravitational wave signals from a large number of astrophysical sources will be present in the LISA data. Information about as many sources as possible must be estimated from time series of strain measurements. Several types of signals are expected t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e960029a239c5ca67025b1f240c3584f
https://doi.org/10.1088/0264-9381/14/6/018
https://doi.org/10.1088/0264-9381/14/6/018
Publikováno v:
Classical and Quantum Gravity. 13:A285-A289
The method for measuring changes in the lengths of the three arms for the LISA gravitational-wave detector is described. Accurate phase measurements are required on signals with Doppler shifts of about 1 MHz for the two main arms of the interferomete
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3e70e1cbc3a1c5c63cac8114bf067778
https://doi.org/10.1088/0264-9381/13/11a/038
https://doi.org/10.1088/0264-9381/13/11a/038
Publikováno v:
AIP Conference Proceedings.
Plans are described to experimentally demonstrate at JILA a possible phase measurement technique for use in LISA interferometry. This demonstration will include use of a compact system for fringe generation and photodetection with realistic beam powe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e928c907955fc076e37af50c9a526b0c
https://doi.org/10.1063/1.57407
https://doi.org/10.1063/1.57407
Autor:
R. T. Stebbins
Publikováno v:
Classical and Quantum Gravity. 26:094014
The LISA science requirements and conceptual design have been fairly stable for over a decade. In the interest of reducing costs, the LISA Project at NASA has looked for simplifications of the architecture, at downsizing of subsystems, and at descope
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b3ead4fe9db863e8f2d23310f84c4ffe
https://doi.org/10.1088/0264-9381/26/9/094014
https://doi.org/10.1088/0264-9381/26/9/094014
Autor:
J. W. Armstrong, P. R. Saulson, R. W. Hellings, Peter L. Bender, R. W. P. Drever, R. T. Stebbins
A Laser‐Interferometer Gravitational‐Wave Observatory (LIGO) is planned for operation in the United States, with two antennas separated by several thousand kilometers. Each antenna would incorporate laser interferometers with 4 km arm lengths, op
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d79641273885330bf09c71ab9662765c
https://resolver.caltech.edu/CaltechAUTHORS:20151223-133541577
https://resolver.caltech.edu/CaltechAUTHORS:20151223-133541577
