Neutron Stars as Probes for the Structure of Compressed Baryonic Matter
Neutron Stars as Probes for the Structure of Compressed Baryonic Matter
批准号:
0854699
负责人:
Fridolin Weber
金额:
$31.5万
依托单位国家:
美国
项目类别:
Standard Grant
财政年份:
2009
资助国家:
美国
项目状态:
已结题
起止时间:
2009-06-15 至 2013-05-31
中文摘要
该奖项是根据2009年美国复苏和再投资法案(公法111-5)资助的。中子星是宇宙中最神秘的物体之一。它们和太阳一样大,但体积却比太阳小一千万亿倍。因此,中子星核心的物质被压缩到比原子核密度大几倍的密度。这一特点,加上观测天文学前所未有的进步,使中子星成为进行广泛有趣的物理研究的极好的天体物理实验室。一些这样的研究是这个NSF项目的主题。这些范围从(1)晶格核之间的核聚变过程和中子星地壳层中物质的新状态的研究到(2)具有比地球磁场强数万亿倍的磁场的中子星的热演化研究。这些研究的结果对于获得新的天体物理仪器投资的全部物理潜力至关重要,例如平方公里阵列(skA)和国际X射线天文台(IXO,以前的星座X),它们承诺发现数万颗中子星。此外,它们为超致密但冷核物质的物理学提供了最有价值的见解,这在相对论对撞机实验中是无法研究的。圣地亚哥地区的中学生和高中生将以公开讲座和多媒体演示的形式从这项研究中受益,这将由研究人员和开展这项项目的学生共同开发。此外,圣地亚哥州立大学的学生将有机会学习并应用先进的量子力学和爱因斯坦广义相对论来进行前沿研究项目,这丰富了他们在课堂上学不到的教育经验。
英文摘要
This award is funded under the American Recovery and Reinvestment Act of 2009 (Public Law 111-5).Neutron stars are among the most enigmatic objects that exist in the Universe. They are as massive as our Sun but are around one thousand trillion times smaller in size. The matter in the cores of neutron stars is therefore compressed to densities that are several times greater than the densities of atomic nuclei. This feature, combined with the unprecedented progress in observational astronomy, makes neutron stars superb astrophysical laboratories for a broad range of intriguing physical studies. Several such studies are the subject of this NSF project. These range from (1) investigations of nuclear fusion processes among lattice nuclei and novel states of matter in the crustal layers of neutron stars to (2) thermal evolution studies of neutron stars possessing magnetic fields that are trillions of times stronger than the Earth's magnetic field. The results of these studies are crucial in order to obtain the full physics potential of the investments that are made in new astrophysical instruments such as the square kilometer Array (skA) and the International X-ray Observatory (IXO, formerly Constellation X), which promise the discovery of tens of thousands of neutron stars. In addition, they provide most valuable insight into the physics of superdense but cold nuclear matter, which can not be studied in relativistic collider experiments.Students from middle and high schools in the San Diego area will profit from this research in the form of public lectures and multimedia presentations, which will be developed by the researches and students carrying out this project. Moreover, students at San Diego State University will get a chance to learn, and apply, advanced quantum mechanics and Einstein's theory of general relativity to cutting-edge research projects, which enriches their educational experience beyond what they learn in the classroom.
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Equations of State of Superdense Nuclear Matter for Use in Neutron Star Merger Simulations
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批准号:2012152
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项目类别:Standard Grant
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资助金额:$31.5万
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财政年份:2020
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负责人:Fridolin Weber
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依托单位:
Quark Matter and its Role in the Evolution of Proton-Neutron Stars to Neutron Stars
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批准号:1714068
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项目类别:Continuing Grant
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资助金额:$27.0万
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财政年份:2017
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负责人:Fridolin Weber
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依托单位:
Astrophysical Studies of Quark Deconfinement
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批准号:1411708
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项目类别:Continuing Grant
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资助金额:$27.0万
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财政年份:2014
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负责人:Fridolin Weber
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依托单位:
Neutron Stars as Probes for the Structure of Dense Nuclear Matter
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批准号:0457329
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项目类别:Continuing Grant
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资助金额:$21.0万
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财政年份:2005
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负责人:Fridolin Weber
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依托单位:
国内基金
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基于STARS分析的渤海营养状态转换及其生态效应研究
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批准号:41906044
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项目类别:青年科学基金项目
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资助金额:25.0万元
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批准年份:2019
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负责人:辛明
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依托单位:
STARS-SRF信号通路在脂代谢中的分子调节机制
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批准号:31171131
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项目类别:面上项目
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资助金额:60.0万元
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批准年份:2011
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负责人:金万洙
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依托单位: