Zugriffsnummer 40682
Dokumenttyp Zeitschriftenartikel
Peer Review mit Peer Review
Sprache Englisch
Titel Influence of polarization and material on Brownian thermal noise of binary grating reflectors
Autor(in); Institution
Dickmann, Johannes; 4.01, Metrologie für funktionale Nanosysteme, PTB-Braunschweig
Rojas Hurtado, Carol Bibiana; 4.01, Metrologie für funktionale Nanosysteme, PTB-Braunschweig
Nawrodt, Ronny; Friedrich-Schiller-Universität Jena, Insitut für Festkörperphysik, Jena, GERMANY
Kroker, Stefanie; 4.01, Metrologie für funktionale Nanosysteme, PTB-Braunschweig; Technische Universität Braunschweig, LENA Laboratory for Emerging Nanometrology, Braunschweig, GERMANY
Quelle/Jahr Physics Letters A: 382 (2018), 33, 2275 - 2281
ISSN 0375-9601 (PRINT) ; 1873-2429 (ONLINE)
DOI
Verlag Amsterdam: Elsevier
Freie Schlagworte Thermal noise ; Grating reflectors ; High precision metrology ; Gravitational wave detection
Zusammenfassung Grating reflectors are a potential low-noise replacement for amorphous multilayer mirrors. We investigate the influence of polarization and refractive index on Brownian thermal noise of binary grating reflectors using Maxwell's stress tensor. Our results demonstrate that the refractive index of the grating material is a critical parameter for thermal noise in these structures. In contrast to multilayer mirrors, a low coating thickness does not necessarily lead to a low thermal noise amplitude for structures with low refractive index. We find that an improved noise performance of grating reflectors requires materials of refractive index ≳2.5. We present a factorized expression for the thermal noise of grating reflectors made of arbitrary materials by simply scaling the noise amplitude with the related material parameters
Themenbereich der Metrologie Nanometrologie

Zitierung

Dickmann, J., Rojas Hurtado, C. B., Nawrodt, R., & Kroker, S. (2018). Influence of polarization and material on Brownian thermal noise of binary grating reflectors. Physics Letters A, 382(33), 2275–2281. https://doi.org/10.1016/j.physleta.2017.07.006

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