Thermal charge carrier driven noise in transmissive semiconductor optics

Autor: Bruns, F. F., Vyatchanin, S. P., Dickmann, J., Glaser, R., Heinert, D., Nawrodt, R., Kroker, S.

Publikováno v: Phys. Rev. D 102, 022006 (2020)

Several sources of noise limit the sensitivity of current gravitational wave detectors. Currently, dominant noise sources include quantum noise and thermal Brownian noise, but future detectors will also be limited by other thermal noise channels. In

Externí odkaz: http://arxiv.org/abs/2003.05345

Brownian Thermal Noise in Functional Optical Surfaces

Autor: Kroker, S., Dickmann, J., Hurtado, C. B. Rojas, Heinert, D., Nawrodt, R., Levin, Y., Vyatchanin, S. P.

Publikováno v: Phys. Rev. D 96, 022002 (2017)

We present a formalism to compute Brownian thermal noise in functional optical surfaces such as grating reflectors, photonic crystal slabs or complex metamaterials. Such computations are based on a specific readout variable, typically a surface integ

Externí odkaz: http://arxiv.org/abs/1705.00157

Scientific Objectives of Einstein Telescope

Autor: Sathyaprakash, B., Abernathy, M., Acernese, F., Ajith, P., Allen, B., Amaro-Seoane, P., Andersson, N., Aoudia, S., Arun, K., Astone, P., Krishnan, B., Barack, L., Barone, F., Barr, B., Barsuglia, M., Bassan, M., Bassiri, R., Beker, M., Beveridge, N., Bizouard, M., Bond, C., Bose, S., Bosi, L., Braccini, S., Bradaschia, C., Britzger, M., Brueckner, F., Bulik, T., Bulten, H. J., Burmeister, O., Calloni, E., Campsie, P., Carbone, L., Cella, G., Chalkley, E., Chassande-Mottin, E., Chelkowski, S., Chincarini, A., Cintio, A. Di., Clark, J., Coccia, E., Colacino, C. N., Colas, J., Colla, A., Corsi, A., Cumming, A., Cunningham, L., Cuoco, E., Danilishin, S., Danzmann, K., Daw, E., Salvo, R. De., Pozzo, W. Del., Dent, T., Rosa, R. De., Fiore, L. Di., Emilio, M. Di. Paolo., Virgilio, A. Di., Dietz, A., Doets, M., Dueck, J., Edwards, M., Fafone, V., Fairhurst, S., Falferi, P., Favata, M., Ferrari, V., Ferrini, F., Fidecaro, F., Flaminio, R., Franc, J., Frasconi, F., Freise, A., Friedrich, D., Fulda, P., Gair, J., Galimberti, M., Gemme, G., Genin, E., Gennai, A., Giazotto, A., Glampedakis, K., Gossan, S., Gouaty, R., Graef, C., Graham, W., Granata, M., Grote, H., Guidi, G., Hallam, J., Hammond, G., Hannam, M., Harms, J., Haughian, K., Hawke, I., Heinert, D., Hendry, M., Heng, I., Hennes, E., Hild, S., Hough, J., Huet, D., Husa, S., Huttner, S., Iyer, B., Jones, D. I., Jones, G., Kamaretsos, I., Mishra, C. Kant, Kawazoe, F., Khalili, F., Kley, B., Kokeyama, K., Kokkotas, K., Kroker, S., Kumar, R., Kuroda, K., Lagrange, B., Lastzka, N., Li, T. G. F., Lorenzini, M., Losurdo, G., Lück, H., Majorana, E., Malvezzi, V., Mandel, I., Mandic, V., Marka, S., Marin, F., Marion, F., Marque, J., Martin, I., Leod, D. Mc., Mckechan, D., Mehmet, M., Michel, C., Minenkov, Y., Morgado, N., Morgia, A., Mosca, S., Moscatelli, L., Mours, B., Müller-Ebhardt, H., Murray, P., Naticchioni, L., Nawrodt, R., Nelson, J., Shaughnessy, R. O'., Ott, C. D., Palomba, C., Paoli, A., Parguez, G., Pasqualetti, A., Passaquieti, R., Passuello, D., Perciballi, M., Piergiovanni, F., Pinard, L., Pitkin, M., Plastino, W., Plissi, M., Poggiani, R., Popolizio, P., Porter, E., Prato, M., Prodi, G., Punturo, M., Puppo, P., Rabeling, D., Racz, I., Rapagnani, P., Re, V., Read, J., Regimbau, T., Rehbein, H., Reid, S., Ricci, F., Richard, F., Robinson, C., Rocchi, A., Romano, R., Rowan, S., Rüdiger, A., Samblowski, A., Santamaría, L., Sassolas, B., Schilling, R., Schmidt, P., Schnabel, R., Schutz, B., Schwarz, C., Scott, J., Seidel, P., Sintes, A. M., Somiya, K., Sopuerta, C. F., Sorazu, B., Speirits, F., Storchi, L., Strain, K., Strigin, S., Sutton, P., Tarabrin, S., Taylor, B., Thürin, A., Tokmakov, K., Tonelli, M., Tournefier, H., Vaccarone, R., Vahlbruch, H., Brand, J. F. J. van. den., Broeck, C. Van. Den., Putten, S. van. der., Veggel, M. van., Vecchio, A., Veitch, J., Vetrano, F., Vicere, A., Vyatchanin, S., Weßels, P., Willke, B., Winkler, W., Woan, G., Woodcraft, A., Yamamoto, K.

Publikováno v: Class. Quantum Grav. 29, 124013, 2012

The advanced interferometer network will herald a new era in observational astronomy. There is a very strong science case to go beyond the advanced detector network and build detectors that operate in a frequency range from 1 Hz-10 kHz, with sensitiv

Externí odkaz: http://arxiv.org/abs/1206.0331

Potential mechanical loss mechanisms in bulk materials for future gravitational wave detectors

Autor: Heinert, D, Grib, A, Haughian, K, Hough, J, Kroker, S, Murray, P, Nawrodt, R, Rowan, S, Schwarz, C, Seidel, P, Tünnermann, A

Publikováno v: J.Phys.Conf.Ser.228:012032,2010

Low mechanical loss materials are needed to further decrease thermal noise in upcoming gravitational wave detectors. We present an analysis of the contribution of Akhieser and thermoelastic damping on the experimental results of resonant mechanical l

Externí odkaz: http://arxiv.org/abs/1003.1613

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