Cryogenics - Revision history

Jan.harms: /* R&D for GW detectors at cryogenic temperatures */

2020-05-26T18:08:34Z

‎R&D for GW detectors at cryogenic temperatures

Jan.harms: /* R&D for GW detectors at cryogenic temperatures */

2020-05-26T18:07:41Z

‎R&D for GW detectors at cryogenic temperatures

Jan.harms: Created page with "= R&D for GW detectors at cryogenic temperatures ="

2020-05-26T17:54:33Z

Created page with "= R&D for GW detectors at cryogenic temperatures ="

New page

= R&D for GW detectors at cryogenic temperatures =

← Older revision		Revision as of 18:08, 26 May 2020
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	= R&D for GW detectors at cryogenic temperatures =		= R&D for GW detectors at cryogenic temperatures =
−	The Einstein Telescope is envisioned in a so-called xylophone configuration, which means that the single-interferometer scheme of the current detectors will be replaced by a pair of interferometers, one operated at room temperature and high laser power, the other at cryogenic temperature and low laser power. Development of new technologies are required to realize an interferometer at low temperature. The current focus is on the development and testing of seismic sensors operating in a cryogenic environment at the National Lab of Gran Sasso (LNGS) in collaboration with a team at Sapienza University of Rome, which leads the cryogenics research in Europe for gravitational-wave detection.	+	The Einstein Telescope is envisioned in a so-called xylophone configuration, which means that the single-interferometer scheme of the current detectors will be replaced by a pair of interferometers, one operated at room temperature and high laser power, the other at cryogenic temperature and low laser power. Development of new technologies are required to realize an interferometer at low temperature. The current focus of our group is on the development and testing of seismic sensors operating in a cryogenic environment at the National Lab of Gran Sasso (LNGS) in collaboration with a team at Sapienza University of Rome, which leads the cryogenics research in Europe for gravitational-wave detection.

← Older revision		Revision as of 18:07, 26 May 2020
Line 1:		Line 1:
	= R&D for GW detectors at cryogenic temperatures =		= R&D for GW detectors at cryogenic temperatures =
		+	The Einstein Telescope is envisioned in a so-called xylophone configuration, which means that the single-interferometer scheme of the current detectors will be replaced by a pair of interferometers, one operated at room temperature and high laser power, the other at cryogenic temperature and low laser power. Development of new technologies are required to realize an interferometer at low temperature. The current focus is on the development and testing of seismic sensors operating in a cryogenic environment at the National Lab of Gran Sasso (LNGS) in collaboration with a team at Sapienza University of Rome, which leads the cryogenics research in Europe for gravitational-wave detection.