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000932844 019__ $$a1155330645$$a1155880318$$a1156747135$$a1157240394$$a1157507107$$a1158321330
000932844 020__ $$a9783030450311$$q(electronic book)
000932844 020__ $$a3030450317$$q(electronic book)
000932844 020__ $$z3030450309
000932844 020__ $$z9783030450304
000932844 0247_ $$a10.1007/978-3-030-45
000932844 0247_ $$a10.1007/978-3-030-45031-1$$2doi
000932844 035__ $$aSP(OCoLC)on1155086938
000932844 035__ $$aSP(OCoLC)1155086938$$z(OCoLC)1155330645$$z(OCoLC)1155880318$$z(OCoLC)1156747135$$z(OCoLC)1157240394$$z(OCoLC)1157507107$$z(OCoLC)1158321330
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000932844 049__ $$aISEA
000932844 050_4 $$aQC174.17.Q33
000932844 08204 $$a530.12$$223
000932844 1001_ $$aCripe, Jonathan.
000932844 24510 $$aBroadband measurement and reduction of quantum radiation pressure noise in the audio band /$$cJonathan Cripe.
000932844 260__ $$aCham :$$bSpringer,$$c2020.
000932844 300__ $$a1 online resource
000932844 336__ $$atext$$btxt$$2rdacontent
000932844 337__ $$acomputer$$bc$$2rdamedia
000932844 338__ $$aonline resource$$bcr$$2rdacarrier
000932844 347__ $$atext file$$bPDF$$2rda
000932844 4901_ $$aSpringer theses
000932844 500__ $$a"Doctoral Thesis accepted by Louisiana State University, L.A., USA."
000932844 504__ $$aIncludes bibliographical references and index.
000932844 5050_ $$aGravitational Waves and Gravitational Wave Detectors -- Optical Springs -- Cantilever Micro-Mirror and Optomechanical Cavity Design -- Radiation-Pressure-Mediated Control of an Optomechanical Cavity -- Observation of an Optical Spring from a Beamsplitter -- Broadband Measurement of Quantum Radiation Pressure Noise at Room Temperature -- Quantum Radiation Pressure Noise Reduction and Evasion -- Future Work and Conclusion.
000932844 506__ $$aAccess limited to authorized users.
000932844 520__ $$aThis book presents a direct measurement of quantum back action, or radiation pressure noise, on a macroscopic object at room temperature across a broad bandwidth in the audio range. This noise source was predicted to be a limitation for gravitational wave interferometers in the 1980s, but it has evaded direct characterization in the gravitational wave community due to the inherent difficult of reducing thermal fluctuations below the quantum back action level. This back action noise is a potential limitation in Advanced LIGO and Advanced Virgo, and Cripes experiment has provided a platform for the demonstration of quantum measurement techniques that will allow quantum radiation pressure noise to be reduced in these detectors. The experimental techniques Cripe developed for this purpose are also applicable to any continuous measurement operating near the quantum limit, and could lead to the possibility of observing non-classical behavior of macroscopic objects.
000932844 650_0 $$aQuantum interference.
000932844 650_0 $$aInterferometers.
000932844 650_0 $$aGravitational waves.
000932844 650_0 $$aElectromagnetic noise.
000932844 77608 $$iPrint version: $$z3030450309$$z9783030450304$$w(OCoLC)1144091654
000932844 830_0 $$aSpringer theses.
000932844 852__ $$bebk
000932844 85640 $$3SpringerLink$$uhttps://univsouthin.idm.oclc.org/login?url=http://link.springer.com/10.1007/978-3-030-45031-1$$zOnline Access$$91397441.1
000932844 909CO $$ooai:library.usi.edu:932844$$pGLOBAL_SET
000932844 980__ $$aEBOOK
000932844 980__ $$aBIB
000932844 982__ $$aEbook
000932844 983__ $$aOnline
000932844 994__ $$a92$$bISE