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Yamaguchi A, Muramatsu H, Hayashi T, Yuasa N, Nakamura K, Takimoto M, Haba H, Konashi K, Watanabe M, Kikunaga H, Maehata K, Yamasaki NY, Mitsuda K. Energy of the ^{229}Th Nuclear Clock Isomer Determined by Absolute γ-ray Energy Difference. Phys Rev Lett 2019; 123:222501. [PMID: 31868403 DOI: 10.1103/physrevlett.123.222501] [Citation(s) in RCA: 11] [Impact Index Per Article: 2.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/18/2019] [Revised: 10/12/2019] [Indexed: 06/10/2023]
Abstract
The low-lying isomeric state of ^{229}Th provides unique opportunities for high-resolution laser spectroscopy of the atomic nucleus. We determine the energy of this isomeric state by taking the absolute energy difference between the excitation energy required to populate the 29.2-keV state from the ground state and the energy emitted in its decay to the isomeric excited state. A transition-edge sensor microcalorimeter was used to measure the absolute energy of the 29.2-keV γ ray. Together with the cross-band transition energy (29.2 keV→ground) and the branching ratio of the 29.2-keV state measured in a recent study, the isomer energy was determined to be 8.30±0.92 eV. Our result is in agreement with the latest measurements based on different experimental techniques, which further confirms that the isomeric state of ^{229}Th is in the laser-accessible vacuum ultraviolet range.
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Affiliation(s)
- A Yamaguchi
- Quantum Metrology Laboratory, RIKEN, Wako, Saitama 351-0198, Japan
| | - H Muramatsu
- Institute of Space and Astronautical Science/Japan Aerospace Exploration Agency, Sagamihara, Kanagawa 252-5210, Japan
| | - T Hayashi
- Institute of Space and Astronautical Science/Japan Aerospace Exploration Agency, Sagamihara, Kanagawa 252-5210, Japan
| | - N Yuasa
- Department of Applied Quantum Physics and Nuclear Engineering, Kyushu University, Fukuoka 819-0395, Japan
| | - K Nakamura
- Safety and Nuclear Security Administration Department, Japan Atomic Energy Agency, Chiyoda-ku, Tokyo 100-8577, Japan
| | - M Takimoto
- Nuclear Fuel Cycle Engineering Laboratories, Japan Atomic Energy Agency, Naka-gun, Ibaraki 319-1194, Japan
| | - H Haba
- Nishina Center for Accelerator-Based Science, RIKEN, Wako, Saitama 351-0198, Japan
| | - K Konashi
- Institute for Materials Research, Tohoku University, Higashiibaraki-gun, Ibaraki 311-1313, Japan
| | - M Watanabe
- Institute for Materials Research, Tohoku University, Higashiibaraki-gun, Ibaraki 311-1313, Japan
| | - H Kikunaga
- Research Center for Electron Photon Science, Tohoku University, Sendai, Miyagi 982-0826, Japan
| | - K Maehata
- Department of Applied Quantum Physics and Nuclear Engineering, Kyushu University, Fukuoka 819-0395, Japan
| | - N Y Yamasaki
- Institute of Space and Astronautical Science/Japan Aerospace Exploration Agency, Sagamihara, Kanagawa 252-5210, Japan
| | - K Mitsuda
- Institute of Space and Astronautical Science/Japan Aerospace Exploration Agency, Sagamihara, Kanagawa 252-5210, Japan
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Eckart ME, Boyce KR, Brown GV, Chiao MP, Fujimoto R, Haas D, den Herder JW, Ishisaki Y, Kelley RL, Kilbourne CA, Leutenegger MA, McCammon D, Mitsuda K, Porter FS, Sawada M, Sneiderman GA, Szymkowiak AE, Takei Y, Tashiro M, Tsujimoto M, de Vries CP, Watanabe T, Yamada S, Yamasaki NY. Calibration of the microcalorimeter spectrometer on-board the Hitomi (Astro-H) observatory (invited). Rev Sci Instrum 2016; 87:11D503. [PMID: 27910640 DOI: 10.1063/1.4961075] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/06/2023]
Abstract
The Hitomi Soft X-ray Spectrometer (SXS) was a pioneering non-dispersive imaging x-ray spectrometer with 5 eV FWHM energy resolution, consisting of an array of 36 silicon-thermistor microcalorimeters at the focus of a high-throughput soft x-ray telescope. The instrument enabled astrophysical plasma diagnostics in the 0.3-12 keV band. We introduce the SXS calibration strategy and corresponding ground calibration measurements that took place from 2012-2015, including both the characterization of the microcalorimeter array and measurements of the x-ray transmission of optical blocking filters.
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Affiliation(s)
- M E Eckart
- NASA Goddard Space Flight Center, Code 662, Greenbelt, Maryland 20771, USA
| | - K R Boyce
- NASA Goddard Space Flight Center, Code 592, Greenbelt, Maryland 20771, USA
| | - G V Brown
- Lawrence Livermore National Laboratory, Livermore, California 94550, USA
| | - M P Chiao
- NASA Goddard Space Flight Center, Code 662, Greenbelt, Maryland 20771, USA
| | - R Fujimoto
- Kanazawa University, Kanazawa, Ishikawa 920-1192, Japan
| | - D Haas
- SRON Netherlands Institute for Space Research, Utrecht, The Netherlands
| | - J-W den Herder
- SRON Netherlands Institute for Space Research, Utrecht, The Netherlands
| | - Y Ishisaki
- Tokyo Metropolitan University, Hachioji, Tokyo 192-0397, Japan
| | - R L Kelley
- NASA Goddard Space Flight Center, Code 662, Greenbelt, Maryland 20771, USA
| | - C A Kilbourne
- NASA Goddard Space Flight Center, Code 662, Greenbelt, Maryland 20771, USA
| | - M A Leutenegger
- NASA Goddard Space Flight Center, Code 662, Greenbelt, Maryland 20771, USA
| | - D McCammon
- University of Wisconsin-Madison, Madison, Wisconsin 53706, USA
| | - K Mitsuda
- Institute of Space and Astronautical Science, JAXA, Sagamihara, Kanagawa 252-5210, Japan
| | - F S Porter
- NASA Goddard Space Flight Center, Code 662, Greenbelt, Maryland 20771, USA
| | - M Sawada
- Aoyama Gakuin University, Sagamihara, Kanagawa 252-5258, Japan
| | - G A Sneiderman
- NASA Goddard Space Flight Center, Code 592, Greenbelt, Maryland 20771, USA
| | | | - Y Takei
- Institute of Space and Astronautical Science, JAXA, Sagamihara, Kanagawa 252-5210, Japan
| | - M Tashiro
- Saitama University, Sakura-ku, Saitama 338-8570, Japan
| | - M Tsujimoto
- Institute of Space and Astronautical Science, JAXA, Sagamihara, Kanagawa 252-5210, Japan
| | - C P de Vries
- SRON Netherlands Institute for Space Research, Utrecht, The Netherlands
| | - T Watanabe
- NASA Goddard Space Flight Center, Code 662, Greenbelt, Maryland 20771, USA
| | - S Yamada
- Tokyo Metropolitan University, Hachioji, Tokyo 192-0397, Japan
| | - N Y Yamasaki
- Institute of Space and Astronautical Science, JAXA, Sagamihara, Kanagawa 252-5210, Japan
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Kikuchi K, Itoh C, Kushino A, Furusho T, Matsushita K, Yamasaki NY, Ohashi T, Fukazawa Y, Ikebe Y, Böhringer H, Matsumoto H. Detection of an X-Ray Hot Region in the Virgo Cluster of Galaxies with ASCA. Astrophys J 2000; 531:L95-L98. [PMID: 10688761 DOI: 10.1086/312535] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
Abstract
Based on mapping observations with ASCA, an unusual hot region with a spatial extent of 1 deg2 was discovered between M87 and M49 at a center coordinate of R.A.=12h27m36s and decl.=9&j0;18' (J2000). The X-ray emission from the region has a 2-10 keV flux of 1x10-11 ergs s-1 cm-2 and a temperature of kT greater, similar4 keV, which is significantly higher than that in the surrounding medium of approximately 2 keV. The internal thermal energy in the hot region is estimated to be VnkT approximately 1060 ergs with a gas density of approximately 10-4 cm-3. A power-law spectrum with a photon index of 1.7-2.3 is also allowed by the data. The hot region suggests there is an energy input due to a shock that is probably caused by the motion of the gas associated with M49, infalling toward the M87 cluster with a velocity greater, similar1000 km s-1.
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