Development of Magnetic Calorimeter for the Search of Intergalactiv Medium by X-Ray Observation

X射线观测寻找间质介质磁量热仪的研制

• 批准号: 12440067
• 负责人: YAMASAKI Noriko
• 金额: $ 9.6万
• 依托单位: The Institute of Space and Astronautical Science (2002)Tokyo Metropolitan University (2000-2001)
• 依托单位国家: 日本
• 项目类别: Grant-in-Aid for Scientific Research (B)
• 财政年份: 2000
• 资助国家: 日本
• 起止时间: 2000 至 2002
• 项目状态: 已结题
• 来源: https://kaken.nii.ac.jp/en/grant/KAKENHI-PROJECT-12440067/
• 关键词: X-Ray Astronomy; Interstellar matter; Intergalactic Medium; micro-calorimeters; Observational Astrophysics; Clusters of Galaxies; 銀河間物; 科学衛星; X線天文; X線分光; 放射線検出器; 極低温; 常磁性体; 磁化率

(1)Measurement of the magnetic properties of 30% Er-doped YAG crustalWe measured the specific heat of 30% Er-doped YAG crustal and derived the magnetic entropy at 93mk〜8K under 8T.(2)Fabrication of the metallic magnetic calorimeter sensorsFabrication process of Er:Au metallic magnetic sensor utilizing IR heater in a vacuum chamber has been established. The concentration of Er were directly measured by RF-SQUID at 4.2K.(3)Setup of SQUID readout at low temperature stageDC-SQUID amplifier for the readout of magnetic calorimeters was introduced at 0.3K stage in a 3He cryostat. Magnetic shield for the SQUID was also set and the SQUID was successfully drived under the magnetic field.(4)Observational and theoretical. studies of the intergalactic medium. We obtained temperature and metal distribution in several cluster of galaxies using ASCA and Chandra observation. The emissivity of oxygen emission line, from warm-hot intergalactic medium were calculated based on the SPH simulation and the detectability by X-ray detectors with high energy resolving power were discussed.

(1)30%Er掺杂YAG地壳磁性能测量测量了30%Er掺杂YAG地壳的比热，并导出了8T下93mk〜8K的磁熵。(2)金属磁量热传感器的制作已经建立了在真空室中利用红外加热器的 Er:Au 金属磁传感器的工艺，并通过 RF-SQUID 直接测量了 Er 的浓度。 4.2K.(3)低温阶段SQUID读出的设置在3He低温恒温器的0.3K阶段引入了用于磁热量计读出的DC-SQUID放大器，并设置了SQUID的磁屏蔽，并成功地在低温下驱动了SQUID。 (4)星系间介质的观测和理论研究，我们利用星系团获得了温度和金属分布。基于SPH模拟计算了ASCA和Chandra观测的暖热星际介质发射氧线的发射率，并讨论了高能分辨X射线探测器的探测能力。

项目成果

H.Ezawa 他8名: "ASCA Observations of the Temperature Structure and Metal Distribution in the Perseus Cluster of Galaxies"Publ.Astron.Soc.Japan. 53-4. 595-604 (2001)

H.Ezawa 和其他 8 人：“ASCA 观测英仙座星系团中的温度结构和金属分布”Publ.Astron.Soc.Japan 53-4 (2001)。

T.Furusho 他8名: "ASCA Temperature Maps of Three Clusters of Galaxies : Abell 1060, AWM 7, and the Centaurus Cluster"Publ.Astron.Soc.Japan. 53-2. 421-432 (2001)

T.Furusho 和其他 8 人：“ASCA 三个星系团的温度图：Abell 1060、AWM 7 和半人马座星系团”Publ.Astron.Soc.Japan 53-2 (2001)。

A.Kushino, et al.: "Erbium-doped yttrium aluminum garnet as a magnetic refrigerant for low temperature X-ray detectors"Journal of Applied Physics. 90. 5812-5818 (2001)

A.Kushino 等人：“掺铒钇铝石榴石作为低温 X 射线探测器的磁性制冷剂”应用物理学杂志。

A.Kushino, et al.: "Study of the X-Ray Background Spectrum and its Large-Scale Fluctuation with ASCA"Publications Astronomical Society of Japan. 54. 327-352 (2002)

A.Kushino 等人：“利用 ASCA 研究 X 射线背景光谱及其大规模波动”，日本天文学会出版物。

Shin Sasaki, Noriko Y.Yamasaki: "Scaling relation to Understand Non-Detection of Cold gas at the Cluster Center"Publ.Astron.Soc.Japan. 54. L1-L5 (2002)

Shin Sasaki、Noriko Y.Yamasaki：“通过缩放关系来理解星团中心未检测到冷气体”Publ.Astron.Soc.Japan。