Zobrazeno 1 - 10
of 41
pro vyhledávání: '"Sneddon, Peter"'
Autor:
Harry, Gregory M., Abernathy, Matthew R., Becerra-Toledo, Andres E., Armandula, Helena, Black, Eric, Dooley, Kate, Eichenfield, Matt, Nwabugwu, Chinyere, Villar, Akira, Crooks, D. R. M., Cagnoli, Gianpietro, Hough, Jim, How, Colin R., MacLaren, Ian, Murray, Peter, Reid, Stuart, Rowan, Sheila, Sneddon, Peter H., Fejer, Martin M, Route, Roger, Penn, Steven D., Ganau, Patrick, Mackowski, Jean-Marie, Michel, Christophe, Pinard, Laurent, Remillieux, Alban
Publikováno v:
Class.Quant.Grav.24:405-416,2007
Reducing thermal noise from optical coatings is crucial to reaching the required sensitivity in next generation interferometric gravitational-waves detectors. Here we show that adding TiO$_2$ to Ta$_2$O$_5$ in Ta$_2$O$_5$/SiO$_2$ coatings reduces the
Externí odkaz:
http://arxiv.org/abs/gr-qc/0610004
Autor:
Penn, Steven D., Sneddon, Peter H., Armandula, Helena, Betzwieser, Joseph C., Cagnoli, Gianpietro, Camp, Jordan, Crooks, D. R. M., Fejer, Martin M., Gretarsson, Andri M., Harry, Gregory M., Hough, Jim, Kittelberger, Scott E., Mortonson, Michael J., Route, Roger, Rowan, Sheila, Vassiliou, Christophoros C.
Publikováno v:
Class.Quant.Grav. 20 (2003) 2917-2928
Current interferometric gravitational wave detectors use test masses with mirror coatings formed from multiple layers of dielectric materials, most commonly alternating layers of SiO2 (silica) and Ta2O5 (tantala). However, mechanical loss in the Ta2O
Externí odkaz:
http://arxiv.org/abs/gr-qc/0302093
Publikováno v:
Open Scholarship of Teaching & Learning; 2022, Vol. 2 Issue 1, p48-58, 11p
Autor:
Sneddon, Peter *
Publikováno v:
In Journal of the Autonomic Nervous System 2000 81(1):218-224
Publikováno v:
5th Annual University of Glasgow Learning and Teaching Conference: Empowering Student Learners in Higher Education
No abstract available.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::53d4ea40160335509e18f1f6155df7da
https://eprints.gla.ac.uk/91955/1/91955.pdf
https://eprints.gla.ac.uk/91955/1/91955.pdf
Autor:
Harry, Gregory M., Armandula, Helena, Black, Eric, Crooks, D. R. M., Cagnoli, Gianpietro, Hough, Jim, Murray, Peter, Reid, Stuart, Rowan, Sheila, Sneddon, Peter, Fejer, Martin M., Route, Roger, Penn, Steve D.
Gravitational waves are a prediction of Einstein's general theory of relativity. These waves are created by massive objects, like neutron stars or black holes, oscillating at speeds appreciable to the speed of light. The detectable effect on the Eart
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od________38::840d3557151672e8e5843c870e1ae1a2
https://resolver.caltech.edu/CaltechAUTHORS:HARao06
https://resolver.caltech.edu/CaltechAUTHORS:HARao06
Autor:
Harry, Gregory M., Armandula, Helena, Black, Eric, Crooks, D. R. M., Cagnoli, Gianpietro, Fejer, Martin M., Hough, Jim, Penn, Steven D., Rowan, Sheila, Route, Roger, Sneddon, Peter
Publikováno v:
Advances in Thin Film Coatings for Optical Applications.
Gravitational waves are a prediction of Einstein's General Theory of Relativity. Astrophysical events like supernova and binary neutron star inspirals are predicted to create potentially detectable waves. The Laser Interferometer Gravitational-wave O
Autor:
Strain, Kenneth A., Allen, B., Aufmuth, P., Aulbert, C., Babak, S., Balasubramanian, R., Barr, B.W., Berukoff, S., Bunkowski, A., Cagnoli, Gianpietro, Cantley, C.A., Casey, M.M., Chelkowski, S., Churches, D., Cokelaer, T., Colacino, C.N., Crooks, David R., Cutler, C., Danzmann, Karsten, Davies, R., Dupuis, Rejean J., Elliffe, E., Fallnich, Carsten, Franzen, A., Freise, A., Gossler, S., Grant, A., Grote, H., Grunewald, S., Harms, J., Heinzel, Gerhard, Heng, Ik S., Hepstonstall, A., Heurs, Michèle, Hewitson, M., Hild, S., Hough, James, Itoh, Y., Jones, R., Huttner, S.H., Kawabe, K., Killow, Christian, Koetter, K., Krishnan, B., Leonhardt, V., Lück, Harald, Machenschalk, B., Malec, M., Mercer, R.A., Messenger, Christopher, Mohanty, S., Mossavi, Kasem, Mukherjee, S., Murray, P., Nagano, S., Newton, G.P., Papa, M.A., Perreur-Lloyd, M., Pitkin, M., Plissi, M.V., Quetschke, V., Re, Virginia, Reid, S., Ribichini, L., Robertson, D.I., Robertson, Norna A., Romano, J.D., Rowan, Sheila, Ruediger, Albrecht, Sathyaprakash, Bangalore S., Schilling, R., Schnabel, R., Schutz, B.F., Seifert, F., Sintes, A.M., Smith, J.R., Sneddon, Peter H., Taylor, I., Taylor, R., Thuering, A., Ungarelli, Carlo, Vahlbruch, H., Vecchio, Alberto, Veitch, J., Ward, Harry, Weiland, U., Welling, Herbert, Williams, P., Willke, Benno, Winkler, Walter, Woan, Graham, Zawischa, Ivo, Sanders, Gary H.
Publikováno v:
Gravitational Wave and Particle Astrophysics Detectors
Proceedings of SPIE ; 5500
Proceedings of SPIE
Proceedings of SPIE ; 5500
Proceedings of SPIE
The GEO 600 laser interferometer with 600 m armlength is part of a worldwide network of gravitational wave detectors. GEO 600 is unique in having advanced multiple pendulum suspensions with a monolithic last stage and in employing a signal recycled o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c01b7d40f666e95089f590d1b0d16ea8
https://www.repo.uni-hannover.de/handle/123456789/12189
https://www.repo.uni-hannover.de/handle/123456789/12189