Astronomy and Astrophysics at Edinburgh
Astronomy and Astrophysics at Edinburgh
批准号:
ST/J001422/1
负责人:
John Peacock
金额:
$382.01万
依托单位:
依托单位国家:
英国
项目类别:
Research Grant
财政年份:
2012
资助国家:
英国
项目状态:
已结题
起止时间:
2012 至 --
中文摘要
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英文摘要
An astonishing feature of modern astrophysical research is that we have in principle a chain of explanation that stretches from processes on cosmological scales of billions of light years, down to the creation of stars, planets around the stars and life on the planets. In a sense, this process is almost a closed loop: the early universe was once of subnuclear scale, so that quantum mechanical uncertainty is bound to seed fluctuations in density, which eventually collapse under gravity to make astronomical structures. This is the same physics of the very small that governs the formation of the atoms out of which we are all made. But unanswered questions abound at all stages of this process. Our theories of the early universe and explanations of its current expansion rest on the concept that empty space can have weight: the so-called "dark energy". We need to study its properties and understand its origin. In so doing, we often assume that Einstein's relativity describes gravity correctly, but can we test this? If the standard theory is correct, dark matter is required, and we are driven to follow the processes by which it clumps, and by which the gas within these clumps evolves, eventally forming stars. New large telescopes on the ground, together with the Hubble Space Telescope, allow us to see this process in action and compare with computer simulations. Nearer to home, we can dissect galaxies such as our own Milky Way into individual stars, for the most detailed view of how they were assembled. And finally we can study how planets arise around these stars, both from new instruments that can measure the presence of "exoplanets" and by computer simulations of how they may be created. Finally, one can ask how life might arise in these early planetary systems, and how it can survive the hostile conditions of outer space.Research in astronomy in Edinburgh attacks all these connected questions. Progress is rapid, and our understanding evolves rapidly. Major progress, even if not final answers, can be expected within a few years. This is an exciting time for our understanding of the universe and our place within it.
期刊论文(9)
专著(0)
科研奖励(0)
会议论文
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DOI:
10.12942/lrr-2013-6
发表时间:
2013
期刊:
Living reviews in relativity
影响因子:
40.6
作者:
[Amendola L, Appleby S, Bacon D, Baker T, Baldi M, Bartolo N, Blanchard A, Bonvin C, Borgani S, Branchini E, Burrage C, Camera S, Carbone C, Casarini L, Cropper M, de Rham C, Di Porto C, Ealet A, Ferreira PG, Finelli F, García-Bellido J, Giannantonio T, Guzzo L, Heavens A, Heisenberg L, Heymans C, Hoekstra H, Hollenstein L, Holmes R, Horst O, Jahnke K, Kitching TD, Koivisto T, Kunz M, La Vacca G, March M, Majerotto E, Markovic K, Marsh D, Marulli F, Massey R, Mellier Y, Mota DF, Nunes NJ, Percival W, Pettorino V, Porciani C, Quercellini C, Read J, Rinaldi M, Sapone D, Scaramella R, Skordis C, Simpson F, Taylor A, Thomas S, Trotta R, Verde L, Vernizzi F, Vollmer A, Wang Y, Weller J, Zlosnik T, Euclid Theory Working Group]
通讯作者:
Euclid Theory Working Group
Identifying clouds over the Pierre Auger Observatory using infrared satellite data
使用红外卫星数据识别皮埃尔奥格天文台上空的云
DOI:
10.1016/j.astropartphys.2013.09.004
发表时间:
2013
期刊:
Astroparticle Physics
影响因子:
3.5
作者:
[Abreu P]
通讯作者:
Abreu P
DOI:
10.1088/0004-637x/769/1/80
发表时间:
2013-05
期刊:
The Astrophysical Journal
影响因子:
--
作者:
[M. Ashby;S. Willner;G. Fazio;J.-S. Huang;R. Arendt;P. Barmby;G. Barro;E. Bell;R. Bouwens]
通讯作者:
M. Ashby;S. Willner;G. Fazio;J.-S. Huang;R. Arendt;P. Barmby;G. Barro;E. Bell;R. Bouwens
The VIMOS Public Extragalactic Redshift Survey (VIPERS) O m 0 from the galaxy clustering ratio measured at z ~ 1?
VIMOS 公共河外红移巡天 (VIPERS) O m 0 从 z ~ 1 处测得的星系簇比?
DOI:
10.1051/0004-6361/201321942
发表时间:
2014
期刊:
Astronomy & Astrophysics
影响因子:
6.5
作者:
[Bel J]
通讯作者:
Bel J
LOFAR detections of low-frequency radio recombination lines towards Cassiopeia A
LOFAR 检测到仙后座 A 的低频射电复合线
DOI:
10.1051/0004-6361/201221001
发表时间:
2013
期刊:
Astronomy & Astrophysics
影响因子:
6.5
作者:
[Asgekar A]
通讯作者:
Asgekar A
共 8 条
Astronomy and Astrophysics at Edinburgh: New Applicants Request
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批准号:ST/L000644/1
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项目类别:Research Grant
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资助金额:$42.3万
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财政年份:2014
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负责人:John Peacock
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依托单位:
Travel support for Edinburgh PATT observers 2010-2012
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批准号:ST/H008594/1
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项目类别:Research Grant
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资助金额:$3.13万
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财政年份:2010
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负责人:John Peacock
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依托单位:
Extragalactic Astronomy and Cosmology at Edinburgh
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批准号:ST/G001979/1
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项目类别:Research Grant
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资助金额:$385.63万
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财政年份:2009
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负责人:John Peacock
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依托单位:
Travel for Edinburgh PATT observers
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批准号:ST/F012292/1
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项目类别:Research Grant
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资助金额:$2.55万
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财政年份:2008
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负责人:John Peacock
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依托单位:
EUCLID Phase A Revised
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批准号:ST/H00310X/1
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项目类别:Research Grant
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资助金额:$7.27万
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财政年份:2008
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负责人:John Peacock
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依托单位:
Genetic Dissection of Synapse Formation in Cell Culture
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批准号:7401379
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项目类别:Standard Grant
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资助金额:$5.0万
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财政年份:1974
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负责人:John Peacock
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依托单位:
国内基金
海外基金
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中英“天体物理(astrophysics)”领域双边研讨会
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批准号:11921003
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项目类别:国际(地区)合作与交流项目
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资助金额:1.5万元
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批准年份:2019
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负责人:常进
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依托单位:
中英“天体物理(astrophysics)”领域双边研讨会
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批准号:11927804
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项目类别:国际(地区)合作与交流项目
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资助金额:1.4万元
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批准年份:2019
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负责人:吴学兵
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依托单位:
中英“天体物理(astrophysics)”领域双边研讨会
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批准号:11981230269
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项目类别:国际(地区)合作与交流项目
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资助金额:1.5万元
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批准年份:2019
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负责人:高亮
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依托单位:
中英“天体物理(astrophysics)”领域双边研讨会
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批准号:--
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项目类别:--
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资助金额:1.8万元
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批准年份:2019
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负责人:林隽
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依托单位:
中英“天体物理(astrophysics)”领域双边研讨会
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批准号:--
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项目类别:--
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资助金额:1.45万元
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批准年份:2019
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负责人:周济林
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依托单位:
中英“天体物理(astrophysics)”领域双边研讨会
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批准号:--
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项目类别:国际(地区)合作与交流项目
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资助金额:1.5万元
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批准年份:2019
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负责人:刘晓为
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依托单位:
中英“天体物理(astrophysics)”领域双边研讨会
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批准号:11973038
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项目类别:国际(地区)合作与交流项目
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资助金额:1.4万元
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批准年份:2019
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负责人:孔旭
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依托单位:
中英“天体物理(astrophysics)”领域双边研讨会
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批准号:--
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项目类别:--
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资助金额:1.5万元
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批准年份:2019
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负责人:王锋
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依托单位:
中英“天体物理(astrophysics)”领域双边研讨会
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批准号:11981230276
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项目类别:国际(地区)合作与交流项目
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资助金额:2万元
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批准年份:2019
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负责人:张双南
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依托单位:
中英“天体物理(astrophysics)”领域双边研讨会
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批准号:--
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项目类别:国际(地区)合作与交流项目
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资助金额:1.5万元
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批准年份:2019
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负责人:韩占文
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依托单位: