Displacement-noise-free interferometeric gravitational-wave detector using unidirectional neutrons with four speeds
Abstract
For further gravitational wave (GW) detections, it is significant to invent a technique to reduce all kinds of mirror displacement noise dominant at low frequencies for ground-based detectors. The neutron displacement-noise-free interferometer (DFI) is one of the tools to reduce all the mirror displacement noise at lower frequencies. In this paper, we describe a further simplified configuration of a neutron DFI in terms of neutron incidence direction. In the new configuration, neutrons enter the interferometer with unidirectional incidence at four speeds as opposed to two bidirectional incidences of opposite directions at two speeds as reported previously. This simplification of the neutron DFI is significant for proof-of-principle experiments.
Additional Information
We would like to thank R. L. Savage for English editing. This work was supported by the Japan Society for the Promotion of Science (JSPS) KAKENHI Grant Number JP19K21875. A. N. is supported by JSPS KAKENHI Grant Nos. JP19H01894 and JP20H04726 and by Research Grants from the Inamori Foundation.Additional details
- Eprint ID
- 118895
- Resolver ID
- CaltechAUTHORS:20230123-451320900.25
- Japan Society for the Promotion of Science (JSPS)
- JP19K21875
- Japan Society for the Promotion of Science (JSPS)
- JP19H01894
- Japan Society for the Promotion of Science (JSPS)
- JP20H04726
- Inamori Foundation
- Created
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2023-02-15Created from EPrint's datestamp field
- Updated
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2023-02-15Created from EPrint's last_modified field
- Caltech groups
- TAPIR