نتایج جستجو برای: sources and detectors

تعداد نتایج: 16854410  

2016
B P Abbott R Abbott T D Abbott M R Abernathy F Acernese K Ackley M Adamo C Adams T Adams P Addesso R X Adhikari V B Adya C Affeldt M Agathos K Agatsuma N Aggarwal O D Aguiar L Aiello A Ain P Ajith B Allen A Allocca P A Altin S B Anderson W G Anderson K Arai M C Araya C C Arceneaux J S Areeda N Arnaud K G Arun S Ascenzi G Ashton M Ast S M Aston P Astone P Aufmuth C Aulbert S Babak P Bacon M K M Bader P T Baker F Baldaccini G Ballardin S W Ballmer J C Barayoga S E Barclay B C Barish D Barker F Barone B Barr L Barsotti M Barsuglia D Barta J Bartlett I Bartos R Bassiri A Basti J C Batch C Baune V Bavigadda M Bazzan B Behnke M Bejger A S Bell C J Bell B K Berger J Bergman G Bergmann C P L Berry D Bersanetti A Bertolini J Betzwieser S Bhagwat R Bhandare I A Bilenko G Billingsley J Birch R Birney S Biscans A Bisht M Bitossi C Biwer M A Bizouard J K Blackburn L Blackburn C D Blair D G Blair R M Blair S Bloemen O Bock T P Bodiya M Boer G Bogaert C Bogan A Bohe P Bojtos C Bond F Bondu R Bonnand B A Boom R Bork V Boschi S Bose Y Bouffanais A Bozzi C Bradaschia P R Brady V B Braginsky M Branchesi J E Brau T Briant A Brillet M Brinkmann V Brisson P Brockill A F Brooks D A Brown D D Brown N M Brown C C Buchanan A Buikema T Bulik H J Bulten A Buonanno D Buskulic C Buy R L Byer L Cadonati G Cagnoli C Cahillane J Calderón Bustillo T Callister E Calloni J B Camp K C Cannon J Cao C D Capano E Capocasa F Carbognani S Caride J Casanueva Diaz C Casentini S Caudill M Cavaglià F Cavalier R Cavalieri G Cella C B Cepeda L Cerboni Baiardi G Cerretani E Cesarini R Chakraborty T Chalermsongsak S J Chamberlin M Chan S Chao P Charlton E Chassande-Mottin S Chatterji H Y Chen Y Chen C Cheng A Chincarini A Chiummo H S Cho M Cho J H Chow N Christensen Q Chu S Chua S Chung G Ciani F Clara J A Clark F Cleva E Coccia P-F Cohadon A Colla C G Collette

On 14 September 2015, a gravitational wave signal from a coalescing black hole binary system was observed by the Advanced LIGO detectors. This paper describes the transient noise backgrounds used to determine the significance of the event (designated GW150914) and presents the results of investigations into potential correlated or uncorrelated sources of transient noise in the detectors around ...

ژورنال: سنجش و ایمنی پرتو 2015

Radon, a progeny of 238U is formed from the radioactive decay of radium. One of the main sources of radon is the emanation from ground water. Radon gas dissolves in groundwater when it moves from the bed of volcanic rocks which contain radioactive elements such as uranium and thorium and then diffuse into spaces. In closed places, the accumulated radon that decays to radioactive particles can c...

Journal: :journal of biomedical physics and engineering 0
s a rahimi tarbiat modares university b hashemi tarbiat modares university s r mahdavi iran university of medical sciences

background: estimating dosimetric parameters for small fields under non-reference conditions leads to significant errors if done based on conventional protocols used for large fields in reference conditions. hence, further correction factors have been introduced to take into account the influence of spectral quality changes when various detectors are used in non-reference conditions at differen...

Journal: :Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 1997

2013
L. Barsotti P. Kwee J. Harms H. Miao

The ongoing global effort to detect gravitational waves continues to push the limits of precision measurement while aiming to provide a new tool for understanding both astrophysics and fundamental physics. Squeezed states of light offer a proven means of increasing the sensitivity of gravitational wave detectors, potentially increasing the rate at which astrophysical sources are detected by mor...

2012
Massimo Cerdonio

The basic physics of g.w.'s emission, propagation and detection is outlined. The general features of candidate sources and detectors are discussed, showing how astrophysical emission events could be detected by devices not far from their Standard Quantum Limit. Two kinds of ground based detectors currently under active development, Km size interferometers and mK cold massive mechanical resonato...

Journal: :IJAHUC 2013
Tsang-Yi Wang Ming-Fong Hsu Jwo-Yuh Wu Jian-Lang Gao

In this paper, the problem of spectrum sensing in cognitive radio communication networks is considered. This paper proposes a robust decision fusion scheme that can perform well when interference caused by other sources is present. Specifically, the proposed detection scheme is based on fusing the local decisions from energy detectors and cyclostationarity-based detectors. The proposed fusion s...

2009
B. S. Sathyaprakash Bernard F. Schutz

Gravitational wave detectors are already operating at interesting sensitivity levels, and they have an upgrade path that should result in secure detections by 2014. We review the physics of gravitational waves, how they interact with detectors (bars and interferometers), and how these detectors operate. We study the most likely sources of gravitational waves and review the data analysis methods...

2010
J. Abadie R. Adhikari E. Amador Ceron P. Barriga L. Barsotti R. Bassiri M. Bastarrika A. Bertolini J. Breyer M. Brinkmann S. Caudill C. Cepeda K. Danzmann R. DeSalvo S. Dhurandhar A. Effler D. Fazi H. Fehrmann M. Flanigan

The Laser Interferometer Gravitational Wave Observatory (LIGO) is a network of three detectors built to detect local perturbations in the space–time metric from astrophysical sources. These detectors, two in Hanford, WA and one in Livingston, LA, are power-recycled Fabry-Perot Michelson interferometers. In their fifth science run (S5), between November 2005 and October 2007, these detectors acc...

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