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Optical cavities for optical atomic ...
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Alvarez, Miguel Dovale.
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Optical cavities for optical atomic clocks, atom interferometry and gravitational-wave detection
Record Type:
Electronic resources : Monograph/item
Title/Author:
Optical cavities for optical atomic clocks, atom interferometry and gravitational-wave detection/ by Miguel Dovale Alvarez.
Author:
Alvarez, Miguel Dovale.
Published:
Cham :Springer International Publishing : : 2019.,
Description:
xxiv, 245 p. :ill., digital ;24 cm.
[NT 15003449]:
Atomic clocks, cold atoms and gravitational waves -- Part 1: Cavities for Optical Atomic Clocks -- Thermal-noise-limited room-temperature ULE cavity -- Isolation from external perturbations -- Measuring resonator stability -- Part 2: Cavities for Atom Interferometry -- Cavity atom optics -- Fundamental limitations of cavity-assisted atom interferometry -- Gravitational wave detection with cavity-assisted atom interferometry -- 4-mirror large-waist cavity with tuneable stability for enhanced atom interferometry -- Part 3: Cavities for Gravitational-wave Detection -- Near-unstable cavities for future gravitational wave detectors -- Modelling parametric instabilities at Advanced LIGO and ET -- Summary and conclusions -- Appendix.
Contained By:
Springer eBooks
Subject:
Atomic clocks. -
Online resource:
https://doi.org/10.1007/978-3-030-20863-9
ISBN:
9783030208639
Optical cavities for optical atomic clocks, atom interferometry and gravitational-wave detection
Alvarez, Miguel Dovale.
Optical cavities for optical atomic clocks, atom interferometry and gravitational-wave detection
[electronic resource] /by Miguel Dovale Alvarez. - Cham :Springer International Publishing :2019. - xxiv, 245 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..
Atomic clocks, cold atoms and gravitational waves -- Part 1: Cavities for Optical Atomic Clocks -- Thermal-noise-limited room-temperature ULE cavity -- Isolation from external perturbations -- Measuring resonator stability -- Part 2: Cavities for Atom Interferometry -- Cavity atom optics -- Fundamental limitations of cavity-assisted atom interferometry -- Gravitational wave detection with cavity-assisted atom interferometry -- 4-mirror large-waist cavity with tuneable stability for enhanced atom interferometry -- Part 3: Cavities for Gravitational-wave Detection -- Near-unstable cavities for future gravitational wave detectors -- Modelling parametric instabilities at Advanced LIGO and ET -- Summary and conclusions -- Appendix.
Devised at the beginning of the 20th century by french physicists Charles Fabry and Alfred Perot, the Fabry-Perot optical cavity is perhaps the most deceptively simple setup in optics, and today a key resource in many areas of science and technology. This thesis delves deeply into the applications of optical cavities in a variety of contexts: from LIGO's 4-km-long interferometer arms that are allowing us to observe the universe in a new way by measuring gravitational waves, to the atomic clocks used to realise time with unprecedented accuracy which will soon lead to a redefinition of the second, and the matterwave interferometers that are enabling us to test and measure gravity in a new scale. The work presented accounts for the elegance and versatility of this setup, which today underpins much of the progress in the frontier of atomic and gravitational experimental physics.
ISBN: 9783030208639
Standard No.: 10.1007/978-3-030-20863-9doiSubjects--Topical Terms:
3300188
Atomic clocks.
LC Class. No.: QB107 / .A48 2019
Dewey Class. No.: 535.470287
Optical cavities for optical atomic clocks, atom interferometry and gravitational-wave detection
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Atomic clocks, cold atoms and gravitational waves -- Part 1: Cavities for Optical Atomic Clocks -- Thermal-noise-limited room-temperature ULE cavity -- Isolation from external perturbations -- Measuring resonator stability -- Part 2: Cavities for Atom Interferometry -- Cavity atom optics -- Fundamental limitations of cavity-assisted atom interferometry -- Gravitational wave detection with cavity-assisted atom interferometry -- 4-mirror large-waist cavity with tuneable stability for enhanced atom interferometry -- Part 3: Cavities for Gravitational-wave Detection -- Near-unstable cavities for future gravitational wave detectors -- Modelling parametric instabilities at Advanced LIGO and ET -- Summary and conclusions -- Appendix.
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Devised at the beginning of the 20th century by french physicists Charles Fabry and Alfred Perot, the Fabry-Perot optical cavity is perhaps the most deceptively simple setup in optics, and today a key resource in many areas of science and technology. This thesis delves deeply into the applications of optical cavities in a variety of contexts: from LIGO's 4-km-long interferometer arms that are allowing us to observe the universe in a new way by measuring gravitational waves, to the atomic clocks used to realise time with unprecedented accuracy which will soon lead to a redefinition of the second, and the matterwave interferometers that are enabling us to test and measure gravity in a new scale. The work presented accounts for the elegance and versatility of this setup, which today underpins much of the progress in the frontier of atomic and gravitational experimental physics.
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Physics and Astronomy (Springer-11651)
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