Optimization of Fabry-Perot optical resonators operated in burst mode for radiation sources-based on Compton scattering (Conference Presentation)

2019 ◽  
Author(s):  
Loïc Amoudry ◽  
Kevin Cassou ◽  
Antoine Courjaud ◽  
Kevin Dupraz ◽  
Titouan Le Barillec ◽  
...  
Keyword(s):  
Compton Scattering ◽  
Optical Resonators ◽  
Burst Mode ◽  
Radiation Sources ◽  
Fabry Perot

scholarly journals Optimization of a Fabry-Perot cavity operated in burst mode for Compton scattering experiments

2018 ◽  
Vol 21 (12) ◽  
Author(s):  
Pierre Favier ◽  
Loïc Amoudry ◽  
Kevin Cassou ◽  
Ronic Chiche ◽  
Kevin Dupraz ◽  
...  
Keyword(s):  
Compton Scattering ◽  
Burst Mode ◽  
Fabry Perot

Optical Resonators and Fabry–Perot Interferometers

1986 ◽  
pp. 444-536
Author(s):  
Salvatore Solimeno ◽  
Bruno Crosignani ◽  
Paolo DiPorto
Keyword(s):  
Optical Resonators ◽  
Fabry Perot

scholarly journals Chiral light in single-handed Fabry-Perot resonators

2021 ◽  
Vol 2015 (1) ◽  
pp. 012012
Author(s):  
Alexey Taradin ◽  
Denis G. Baranov
Keyword(s):  
Circular Dichroism ◽  
Standing Wave ◽  
Optical Cavity ◽  
Optical Resonators ◽  
Resonant Excitation ◽  
Length Scales ◽  
Optical Cavities ◽  
Fabry Perot ◽  
Vacuum States ◽  
Circular Dichroïsm

Abstract Chirality is a universal phenomenon that is encountered on many different length scales in nature. Interaction of chiral matter with chiral light results in the effect of circular dichroism, which underlies many techniques of discriminating molecular enantiomers. Enhancing dichroic effects is typically achieved by interfacing chiral matter with various optical resonators. In this context it is important to understand how the eigenmodes of optical cavities relate to the field states with well-defined handedness. Here, we present the model of a single-handedness chiral optical cavity supporting only an eigenmode of a given handedness without the presence of modes of other helicity. Resonant excitation of the cavity with light of appropriate handedness enables formation of a helical standing wave with a uniform chirality density, while the opposite handedness does not cause any resonant effects. Our findings expand the set of tools for investigations of chiral matter and open the door towards studies of chiral electromagnetic vacuum states.

scholarly journals Compact x-ray source based on burst-mode inverse Compton scattering at 100 kHz

2014 ◽  
Vol 17 (12) ◽  
Author(s):  
W. S. Graves ◽  
J. Bessuille ◽  
P. Brown ◽  
S. Carbajo ◽  
V. Dolgashev ◽  
...  
Keyword(s):  
Compton Scattering ◽  
X Ray ◽  
Burst Mode ◽  
Inverse Compton Scattering ◽  
Inverse Compton

scholarly journals Fabry-Perot description for Mie resonances of rectangular dielectric nanowire optical resonators

2016 ◽  
Vol 24 (26) ◽  
pp. 29760 ◽  
Author(s):  
Patrick E. Landreman ◽  
Hamidreza Chalabi ◽  
Junghyun Park ◽  
Mark L. Brongersma
Keyword(s):  
Optical Resonators ◽  
Fabry Perot

scholarly journals Information-Measuring Complex to Detect High Frequency Gravitational Waves

2021 ◽  
pp. 13-23
Author(s):  
I. S. Golyak ◽  
A. N. Morozov ◽  
A. L. Nazolin ◽  
S. E. Tabalin ◽  
A. A. Esakov ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Gravitational Waves ◽  
High Frequency ◽  
Low Frequency ◽  
Optical Resonators ◽  
Integer Number ◽  
Optical Scheme ◽  
Gravitational Antenna ◽  
Optical Resonance ◽  
Fabry Perot

The gravitational waves predicted by the general theory of relativity and detected by the Laser Interferometer Gravitational-wave Observatory (LIGO) have typical frequencies in the range of 30 ... 300 Hz. Current theories of gravity predict the existence of high-frequency gravitational waves with frequencies of 10 ... 100 MHz, including those of cosmological origin, induced by quantum fluctuations of the scalar field at the stage of cosmological inflation in the early Universe.Multi-beam optical resonators, in particular the Fabry-Perot interferometers, can be used to detect high-frequency gravitational waves. When using multi-beam optical resonators, it is possible to use the phenomenon of low-frequency optical resonance, which allows us to have a selective response to the gravitational wave effect. The gravitational-optical resonance in a multi-beam interferometer occurs if the condition is fulfilled that an integer number of half-waves of gravitational radiation is along the length of the resonator.The use of a multi-beam interferometer to detect high-frequency gravitational waves does not require the creation of a complex system for decoupling mirrors used for gravitational antennas operating in the low-frequency part of the spectrum. This is due to the fact that the frequency of mechanical vibrations of the interferometer mirrors is significantly less than the frequency of the gravitational wave.The paper considers possible optical schemes of a high-frequency gravitational antenna: based on the traditional Michelson interferometer, in the arms of which two Fabry-Perot interferometers are available, and on the basis of the Mach-Zehnder optical scheme, where Fabry-Perot interferometers can be made in the form of two perpendicular arms, with reflecting mirrors at the bend of the beam. The advantage of the second scheme is that three photo-detectors, one being main and two others being auxiliary, can be used, and there is a possibility to detect radiation transmitted by Fabry-Perot interferometers.To prove that detection of high-frequency gravitational waves is possible, a potential sensitivity of the high-frequency gravitational antenna has been estimated in the paper.

Brillouin Scattering in Liquids at 4416 Å and 4765 Å

1973 ◽  
Vol 28 (7) ◽  
pp. 1152-1155
Author(s):  
Silas E. Gustafsson ◽  
H. E. Gunilla Knape ◽  
Lena M. Torell
Keyword(s):  
Brillouin Scattering ◽  
Organic Liquids ◽  
Thermal Waves ◽  
Frequency Shifts ◽  
Radiation Sources ◽  
Fabry Perot ◽  
Stokes Lines ◽  
Ion Laser ◽  
Anti Stokes ◽  
Argon Ion

An argon ion laser operating at 4765 Å and a helium-cadmium laser operating at 4416 Å have been used as radiation sources to study Brillouin scattering in seven organic liquids. The Brillouin spectra were investigated at 90° with a pressure scanned Fabry-Perot spectrometer. The measured frequency shifts between the Stokes and anti-Stokes lines were used to determine the hypersonic velocities of thermal waves at frequencies between 4.8 and 7.2 GHz. No dispersion of the hypersound could be detected.

Doubly-Resonant Fabry-Perot Cavity for Power Enhancement of Burst-Mode Picosecond Ultraviolet Pulses

CLEO: 2015 ◽  
2015 ◽  
Author(s):  
Abdurahim Rakhman ◽  
Chunning Huang ◽  
Mark Notcutt ◽  
Yun Liu
Keyword(s):  
Burst Mode ◽  
Power Enhancement ◽  
Fabry Perot
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