Search Results - "Affeldt, Christoph"
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Direct limits for scalar field dark matter from a gravitational-wave detector
Published in Nature (London) (16-12-2021)“…The nature of dark matter remains unknown to date, although several candidate particles are being considered in a dynamically changing research landscape 1 …”
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First Demonstration of 6 dB Quantum Noise Reduction in a Kilometer Scale Gravitational Wave Observatory
Published in Physical review letters (29-01-2021)“…Photon shot noise, arising from the quantum-mechanical nature of the light, currently limits the sensitivity of all the gravitational wave observatories at…”
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Characterization and evasion of backscattered light in the squeezed-light enhanced gravitational wave interferometer GEO 600
Published in Optics express (06-11-2023)“…Squeezed light is injected into the dark port of gravitational wave interferometers, in order to reduce the quantum noise. A fraction of the interferometer…”
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High power and ultra-low-noise photodetector for squeezed-light enhanced gravitational wave detectors
Published in Optics express (05-09-2016)“…Current laser-interferometric gravitational wave detectors employ a self-homodyne readout scheme where a comparatively large light power (5-50 mW) is detected…”
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GW170817: Implications for the stochastic gravitationnal-wave background from compact binary coalescences
Published in Physical review letters (2018)“…The LIGO Scientific and Virgo Collaborations have announced the event GW170817, the first detection of gravitational waves from the coalescence of two neutron…”
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GEO600 beam splitter thermal compensation system: new design and commissioning
Published 05-08-2024“…Gravitational waves have revolutionised the field of astronomy by providing scientists with a new way to observe the universe and gain a better understanding…”
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First demonstration of neural sensing and control in a kilometer-scale gravitational wave observatory
Published 15-01-2023“…Suspended optics in gravitational wave (GW) observatories are susceptible to alignment perturbations, particularly slow drifts over time, due to variations in…”
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8
Characterization and evasion of backscattered light in the squeezed-light enhanced gravitational wave interferometer GEO 600
Published 29-05-2023“…Squeezed light is injected into the dark port of gravitational wave interferometers, in order to reduce the quantum noise. A fraction of the interferometer…”
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9
Bilinear noise subtraction at the GEO 600 observatory
Published 28-05-2020“…Phys. Rev. D 101, 102006 (2020) Longitudinal control signals used to keep gravitational wave detectors at a stable operating point are often affected by…”
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10
Direct limits for scalar field dark matter from a gravitational-wave detector
Published 18-10-2021“…The nature of dark matter remains unknown to date; several candidate particles are being considered in a dynamically changing research landscape. Scalar field…”
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11
First demonstration of 6 dB quantum noise reduction in a kilometer scale gravitational wave observatory
Published 20-05-2020“…Phys. Rev. Lett. 126, 041102 (2021) Photon shot noise, arising from the quantum-mechanical nature of the light, currently limits the sensitivity of all the…”
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12
Matrix Heater in the Gravitational Wave Observatory GEO 600
Published 04-06-2018“…Large scale laser interferometric gravitational wave detectors (GWDs), such as GEO 600 require high quality optics to reach their design sensitivity. The…”
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Phase Control of Squeezed Vacuum States of Light in Gravitational Wave Detectors
Published 13-11-2014“…Quantum noise will be the dominant noise source for the advanced laser interferometric gravitational wave detectors currently under construction…”
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14
Alignment sensing and control for squeezed vacuum states of light
Published 23-07-2015“…Beam alignment is an important practical aspect of the application of squeezed states of light. Misalignments in the detection of squeezed light result in a…”
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15
Thermal Correction of Astigmatism in the Gravitational Wave Observatory GEO 600
Published 21-11-2013“…The output port of GEO 600 is dominated by unwanted high order modes (HOMs). The current thermal actuation system, a ring heater behind one of the folding…”
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