课题基金 / 基金详情

Astrophysics at the University of Birmingham - Consolidated grant 2022-2025

Astrophysics at the University of Birmingham - Consolidated grant 2022-2025
伯明翰大学天体物理学 - 综合赠款 2022-2025
批准号:
ST/W000946/1
负责人:
Alberto Vecchio
金额:
$126.93万
依托单位:
依托单位国家:
英国
项目类别:
Research Grant
财政年份:
2022
资助国家:
英国
项目状态:
未结题
起止时间:
2022 至 --

项目摘要

项目成果

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中文摘要
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英文摘要
The Universe looks very different depending on how we observe it. The use of a broad range of cosmic messengers, the full spectrum of "electromagnetic radiation" - ranging from radio waves through infrared radiation and light, to X-rays and gamma rays - and, as of only a few years ago also ripples in space and time known as gravitational waves reveal that the Universe is not a quiet place. It is characterised by violent and dramatic phenomena, powerful explosions that produce astonishingly large mount of energy over short periods of time. We can now study many of these catastrophic events in great detail thanks to a large range of superb observatories, some of which coming on-line in the next couple of years. We may be very surprised yet again, and discover new phenomena.Our programme looks at some of the most exciting transient phenomena from many different angles and has black holes and extreme ("compact") objects at its centre. We aim to study how black holes devour and shred stars at the centre of galaxies. We will use the effect of bending of light over cosmic scales to observe through massive lenses - groups and clusters of galaxies - multiple images of some of these catastrophic events, gain new insights about their engines and how the Universe evolves as a whole. We will also try to "hear" for the very first time the cosmic whisper of the population of billion solar mass black holes paring up at the centre of galaxies and radiating gravitational waves. We believe we can detect this radiation now with powerful galactic scale "instruments", the ultra-stable clocks provided to us by radio lighthouses known as pulsars. If this happens, we would open a new observational window on the Universe.Black holes are also spectacularly simple objects. They are a sort of fundamental particle of gravity and testing their properties is of paramount importance. Using the many binary black holes that we now routinely observe with gravitational-wave laser interferometers we will test to unprecedented accuracy one of the most famous predictions surrounding these objects: Hawking's horizon area theorem.Most or all of the cosmic explosions that we have described above take place in galaxies, which astronomers have studied in great detail for many decades. However, how galaxies form and evolve as part of the tangled structures in the Universe known as "the cosmic web" is still surrounded by mystery. New powerful surveys using some of the best telescopes in the world will allow us to put existing theoretical models under test, and we will gain new insights about galaxy evolution over cosmic time and the myriad of interlinked physical processes that take place in these environments.
期刊论文(10)
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会议论文
The NANOGrav 15 yr Data Set: Detector Characterization and Noise Budget
NANOGrav 15 年数据集:探测器特征和噪声预算
DOI: 10.3847/2041-8213/acda88
发表时间: 2023
期刊: The Astrophysical Journal Letters
影响因子: --
作者: [Agazie, Gabriella, Anumarlapudi, Akash, Archibald, Anne M., Arzoumanian, Zaven, Baker, Paul T., Bécsy, Bence, Blecha, Laura, Brazier, Adam, Brook, Paul R., Burke-Spolaor, Sarah]
通讯作者: Burke-Spolaor, Sarah
DOI: 10.3847/2041-8213/ace18b
发表时间: 2023-06
期刊: The Astrophysical Journal Letters
影响因子: --
作者: [G. Agazie;A. Anumarlapudi;A. Archibald;P. Baker;B. B'ecsy;L. Blecha;Alexander Bonilla;A. Brazier;P. Brook;S. Burke-Spolaor;R. Burnette;R. Case;J. A. Casey-Clyde;M. Charisi;S. Chatterjee;K. Chatziioannou;B. Cheeseboro;Siyuan Chen;T. Cohen;J. Cordes;N. Cornish;F. Crawford;H. Cromartie;K. Crowter;C. Cutler;D. D’Orazio;M. DeCesar;D. DeGan;P. Demorest;Heling Deng;T. Dolch;B. Drachler;E. Ferrara;W. Fiore;E. Fonseca;G. Freedman;E. Gardiner;N. Garver-Daniels;P. Gentile;K. A. Gersbach;J. Glaser;D. Good;K. Gultekin;J. Hazboun;S. Hourihane;K. Islo;R. Jennings;A. Johnson;Megan L. Jones;A. Kaiser;D. Kaplan;L. Kelley;M. Kerr;J. Key;N. Laal;M. Lam;W. Lamb;T. Lazio;N. Lewandowska;T. Littenberg;Tianyu Liu;Jing Luo;R. Lynch;Chung-Pei Ma;D. Madison;A. McEwen;J. McKee;M. Mclaughlin;N. McMann;B. W. Meyers;P. Meyers;C. Mingarelli;A. Mitridate;P. Natarajan;C. Ng;D. Nice;S. Ocker;K. Olum;T. Pennucci;B. Perera;P. Petrov;N. Pol;H. Radovan;S. Ransom;P. Ray;J. Romano;J. Runnoe;S. C. Sardesai;A. Schmiedekamp;C. Schmiedekamp;K. Schmitz;L. Schult;B. Shapiro-Albert;X. Siemens;J. Simon;M. Siwek;I. Stairs;D. Stinebring;K. Stovall;Jerry P. Sun;A. Susobhanan;J. Swiggum;Jacob M. Taylor;S. Taylor;J. E. Turner;C. Unal;M. Vallisneri;S. Vigeland;Jeremy M. Wachter;H. Wahl;Qiaohong Wang;C. Witt;David Wright;O. Young]
通讯作者: G. Agazie;A. Anumarlapudi;A. Archibald;P. Baker;B. B'ecsy;L. Blecha;Alexander Bonilla;A. Brazier;P. Brook;S. Burke-Spolaor;R. Burnette;R. Case;J. A. Casey-Clyde;M. Charisi;S. Chatterjee;K. Chatziioannou;B. Cheeseboro;Siyuan Chen;T. Cohen;J. Cordes;N. Cornish;F. Crawford;H. Cromartie;K. Crowter;C. Cutler;D. D’Orazio;M. DeCesar;D. DeGan;P. Demorest;Heling Deng;T. Dolch;B. Drachler;E. Ferrara;W. Fiore;E. Fonseca;G. Freedman;E. Gardiner;N. Garver-Daniels;P. Gentile;K. A. Gersbach;J. Glaser;D. Good;K. Gultekin;J. Hazboun;S. Hourihane;K. Islo;R. Jennings;A. Johnson;Megan L. Jones;A. Kaiser;D. Kaplan;L. Kelley;M. Kerr;J. Key;N. Laal;M. Lam;W. Lamb;T. Lazio;N. Lewandowska;T. Littenberg;Tianyu Liu;Jing Luo;R. Lynch;Chung-Pei Ma;D. Madison;A. McEwen;J. McKee;M. Mclaughlin;N. McMann;B. W. Meyers;P. Meyers;C. Mingarelli;A. Mitridate;P. Natarajan;C. Ng;D. Nice;S. Ocker;K. Olum;T. Pennucci;B. Perera;P. Petrov;N. Pol;H. Radovan;S. Ransom;P. Ray;J. Romano;J. Runnoe;S. C. Sardesai;A. Schmiedekamp;C. Schmiedekamp;K. Schmitz;L. Schult;B. Shapiro-Albert;X. Siemens;J. Simon;M. Siwek;I. Stairs;D. Stinebring;K. Stovall;Jerry P. Sun;A. Susobhanan;J. Swiggum;Jacob M. Taylor;S. Taylor;J. E. Turner;C. Unal;M. Vallisneri;S. Vigeland;Jeremy M. Wachter;H. Wahl;Qiaohong Wang;C. Witt;David Wright;O. Young
DOI: 10.3847/2041-8213/acdac6
发表时间: 2023-06
期刊: The Astrophysical Journal Letters
影响因子: --
作者: [G. Agazie;A. Anumarlapudi;A. Archibald;Z. Arzoumanian;P. Baker;B. Bécsy;L. Blecha;A. Brazier;P. Brook;S. Burke-Spolaor;R. Burnette;R. Case;M. Charisi;S. Chatterjee;K. Chatziioannou;B. Cheeseboro;Siyuan Chen;T. Cohen;J. Cordes;N. Cornish;F. Crawford;H. Cromartie;K. Crowter;C. Cutler;M. DeCesar;D. DeGan;P. Demorest;Heling Deng;T. Dolch;B. Drachler;J. Ellis;E. Ferrara;W. Fiore;E. Fonseca;G. Freedman;N. Garver-Daniels;P. Gentile;K. A. Gersbach;J. Glaser;D. Good;K. Gultekin;J. Hazboun;S. Hourihane;K. Islo;R. Jennings;A. Johnson;Megan L. Jones;A. Kaiser;D. Kaplan;L. Kelley;M. Kerr;J. Key;T. C. Klein;N. Laal;M. Lam;W. Lamb;T. Lazio;N. Lewandowska;T. Littenberg;Tianyu Liu;A. Lommen;D. Lorimer;Jing Luo;R. Lynch;Chung-Pei Ma;D. Madison;M. A. Mattson;A. McEwen;J. McKee;M. Mclaughlin;N. McMann;B. W. Meyers;P. Meyers;C. Mingarelli;A. Mitridate;P. Natarajan;C. Ng;D. Nice;S. Ocker;K. Olum;T. Pennucci;B. Perera;P. Petrov;N. Pol;H. Radovan;S. Ransom;P. Ray;J. Romano;S. C. Sardesai;A. Schmiedekamp;C. Schmiedekamp;K. Schmitz;L. Schult;B. Shapiro-Albert;X. Siemens;J. Simon;M. Siwek;I. Stairs;D. Stinebring;K. Stovall;Jerry P. Sun;A. Susobhanan;J. Swiggum;Jacob M. Taylor;S. Taylor;J. E. Turner;C. Unal;M. Vallisneri;R. V. Haasteren;S. Vigeland;H. Wahl;Qiaohong Wang;C. Witt;O. Young]
通讯作者: G. Agazie;A. Anumarlapudi;A. Archibald;Z. Arzoumanian;P. Baker;B. Bécsy;L. Blecha;A. Brazier;P. Brook;S. Burke-Spolaor;R. Burnette;R. Case;M. Charisi;S. Chatterjee;K. Chatziioannou;B. Cheeseboro;Siyuan Chen;T. Cohen;J. Cordes;N. Cornish;F. Crawford;H. Cromartie;K. Crowter;C. Cutler;M. DeCesar;D. DeGan;P. Demorest;Heling Deng;T. Dolch;B. Drachler;J. Ellis;E. Ferrara;W. Fiore;E. Fonseca;G. Freedman;N. Garver-Daniels;P. Gentile;K. A. Gersbach;J. Glaser;D. Good;K. Gultekin;J. Hazboun;S. Hourihane;K. Islo;R. Jennings;A. Johnson;Megan L. Jones;A. Kaiser;D. Kaplan;L. Kelley;M. Kerr;J. Key;T. C. Klein;N. Laal;M. Lam;W. Lamb;T. Lazio;N. Lewandowska;T. Littenberg;Tianyu Liu;A. Lommen;D. Lorimer;Jing Luo;R. Lynch;Chung-Pei Ma;D. Madison;M. A. Mattson;A. McEwen;J. McKee;M. Mclaughlin;N. McMann;B. W. Meyers;P. Meyers;C. Mingarelli;A. Mitridate;P. Natarajan;C. Ng;D. Nice;S. Ocker;K. Olum;T. Pennucci;B. Perera;P. Petrov;N. Pol;H. Radovan;S. Ransom;P. Ray;J. Romano;S. C. Sardesai;A. Schmiedekamp;C. Schmiedekamp;K. Schmitz;L. Schult;B. Shapiro-Albert;X. Siemens;J. Simon;M. Siwek;I. Stairs;D. Stinebring;K. Stovall;Jerry P. Sun;A. Susobhanan;J. Swiggum;Jacob M. Taylor;S. Taylor;J. E. Turner;C. Unal;M. Vallisneri;R. V. Haasteren;S. Vigeland;H. Wahl;Qiaohong Wang;C. Witt;O. Young
The NANOGrav 15-Year Data Set: Detector Characterization and Noise Budget
NANOGrav 15 年数据集:探测器特征和噪声预算
DOI: 10.48550/arxiv.2306.16218
发表时间: 2023
期刊:
影响因子: --
作者: [Agazie G]
通讯作者: Agazie G
8
    Gravitational wave science at the University of Birmingham
    • 批准号:
      ST/V005677/1
    • 项目类别:
      Research Grant
    • 资助金额:
      $114.02万
    • 财政年份:
      2021
    • 负责人:
      Alberto Vecchio
    • 依托单位:
    Advanced LIGO Operations Support
    • 批准号:
      ST/V001167/1
    • 项目类别:
      Research Grant
    • 资助金额:
      $13.4万
    • 财政年份:
      2020
    • 负责人:
      Alberto Vecchio
    • 依托单位:
    Astrophysics at the University of Birmingham
    • 批准号:
      ST/S000305/1
    • 项目类别:
      Research Grant
    • 资助金额:
      $234.1万
    • 财政年份:
      2019
    • 负责人:
      Alberto Vecchio
    • 依托单位:
    Astrophysics at the University of Birmingham: Consolidated Grant 2016-2019
    • 批准号:
      ST/N000633/1
    • 项目类别:
      Research Grant
    • 资助金额:
      $240.06万
    • 财政年份:
      2016
    • 负责人:
      Alberto Vecchio
    • 依托单位:
    海外基金