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The Laser Interferometer Gravitational-Wave Observatory (LIGO) Local Educational Outreach Partnership

The Laser Interferometer Gravitational-Wave Observatory (LIGO) Local Educational Outreach Partnership
激光干涉仪引力波天文台 (LIGO) 当地教育推广合作伙伴关系
批准号:
0355471
负责人:
VerJanis Peoples
金额:
$0.0万
依托单位:
依托单位国家:
美国
项目类别:
Cooperative Agreement
财政年份:
2004
资助国家:
美国
项目状态:
已结题
起止时间:
2004-04-01 至 2010-03-31

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中文摘要
翻译
这个合作奖给加州理工学院和南方大学巴吞鲁日。它使游客中心的发展在利文斯顿,洛杉矶网站的激光干涉引力波天文台(LIGO)。该中心将包含动手展品,描绘LIGO运作的物理科学方面,其引力波的目标来源,以及对其数据的分析和解释。展览将与旧金山弗朗西斯科合作提供。该中心及其展品将为南方大学巴吞鲁日(SUBR)的职前和在职科学教师培训提供重点。路易斯安那州摄政委员会将通过现有计划LaSIP和LA GEARUP协调教师和学生前往中心和SUBR的交通,以最大限度地让中心相关活动接触到服务不足的群体。此外,SUBR物理和教育专业的学生和博士后将接受培训,担任该中心的讲师。LIGO的目标是直接探测引力波,开创引力波天文学。LIGO由加州理工学院(与麻省理工学院合作)通过与NSF的合作协议运营。LIGO科学合作组织由8个国家40多个机构的约450名科学家组成。LIGO已经在运行和获取数据,同时继续完善其仪器以达到其设计灵敏度。LIGO仪器的工作原理是测量由引力波通过引起的仪器干涉仪反射镜之间距离的微小变化。LIGO已经可以测量小于原子核直径百分之一的变化--在设计目标的十倍之内。引力波被认为是由宇宙中最剧烈的事件产生的,包括黑洞和中子星的形成和合并,超新星以及大爆炸本身。LIGO的科学,涉及许多公众已经知道的物理学方面-爱因斯坦,黑洞,爆炸的恒星,大爆炸-已经引起了公众的兴趣。利用LIGO科学和SUBR的科学教育计划来激励物理科学的教学和学习,特别是在像路易斯安那州这样服务不足的地区,可以为类似大型项目的推广和教育活动提供重要的模式。该奖项由物理部和数学和物理科学理事会多学科活动办公室共同资助。
英文摘要
This collaborative award to the California Institute of Technology and to Southern University Baton Rouge. It enables the development of a Visitor Center at the Livingston, LA site of the Laser Interferometer Gravitational-wave Observatory (LIGO). The Center will contain hands-on exhibits depicting aspects of physical science underlying the functioning of LIGO, its target sources of gravitational waves, and the analysis and interpretation of its data. The exhibits will be provided in collaboration with the Exploratorium of San Francisco. The Center and its exhibits will then provide the focus for revamped pre-service and in-service science teacher training at Southern University Baton Rouge (SUBR). The Louisiana Board of Regents, through existing programs LaSIP and LA GEARUP, will coordinate transportation of teachers and students to the Center and to SUBR to maximize the exposure of Center-related activities to underserved groups. In addition, SUBR physics and education students and postdocs will be trained to serve as docents at the Center. LIGO's goal is the direct detection of gravitational waves and the initiation of gravitational wave astronomy. LIGO is operated by Caltech (with subcontract to MIT) through a cooperative agreement with NSF. The LIGO Scientific Collaboration comprises approximately 450 scientists in over 40 institutions in 8 countries. LIGO is already operating and taking data while continuing to refine its instrumentation to reach its design sensitivity. The LIGO instruments work by measuring exquisitely tiny changes in the distances between the mirrors of the instruments' interferometers caused by the passage of gravitational waves. LIGO can already measure changes smaller than one one-hundredth the diameter of the atomic nucleus---within a factor of ten of the design goal. Gravitational waves are expected to be produced by the universe's most violent events including the formation and mergers of black holes and neutron stars, supernovae, and the Big Bang itself. LIGO's science, involving many of those aspects of physics already known to the general public---Einstein, black holes, exploding stars, the big bang---has already captured the public's interest. Leveraging LIGO science and SUBR's science education programs to motivate teaching and learning of physical science, especially in an underserved area like Louisana, could provide an important model for the outreach and educational activities of similar large projects.This award is co-funded by the Physics Division and the Office of Multidisciplinary Activities in the Mathematical and Physical Sciences Directorate.
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