课题基金 / 基金详情

Cosmology and Astrophysics at Portsmouth

Cosmology and Astrophysics at Portsmouth
朴茨茅斯的宇宙学和天体物理学
批准号:
ST/N000668/1
负责人:
Robert Nichol
金额:
$208.57万
依托单位:
依托单位国家:
英国
项目类别:
Research Grant
财政年份:
2016
资助国家:
英国
项目状态:
已结题
起止时间:
2016 至 --

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项目成果

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中文摘要
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英文摘要
This consolidated grant is to support cosmologists and astrophysicists in the Institute of Cosmology and Gravitation (ICG) at the University of Portsmouth. The ICG was formed in 2002 through a strategic investment from the university, and now hosts 50 researchers making it one of the largest extragalactic astronomy groups in the UK e.g. ranked 8th in research outputs in the recent REF2014.Cosmology and astrophysics are experiencing a golden age of discovery driven by new experiments and theoretical advances. However, we still face three fundamental challenges before a more complete model of the Universe can be achieved: i) What are the properties of the "dark matter" and "dark energy" that make up 96% of the Universe? ii) How do galaxies form and evolve? iii) What is the origin, and statistical nature, of structures in the Universe? This grant will address these fundamental problems through pioneering theoretical work and the use of new surveys of the sky to map billions of distant galaxies. Galaxies are the "building blocks" of the Universe and as well as studying how they form, we will use the galaxies to improve our understanding of cosmology (the properties of the Universe as a whole). We will exploit current and forthcoming galaxy surveys including the Dark Energy Survey, SDSS-IV, SERVS and Euclid to measure numerous probes of cosmology such as the clustering of galaxies, supernovae and weak gravitational lensing (distortions of the galaxies' shape due to gravity). Precise cosmological models will be constructed and analysed, and simulated with Portsmouth's SCIAMA supercomputer. These models will be compared to data to reveal the cosmological properties of the Universe. The surveys will be used to study how galaxies form, by measuring their colours and taking detailed spectra of the galaxies. We will also study the evolution of galaxies by comparing the galaxies in the nearby Universe, showing their present state, with those of the distant Universe, which gives us a window into the past.Bringing together all our work, we will model and measure the evolution of the Universe throughout its entire history. We will study how quantum fluctuations in the very early universe may be stretched by inflation in the very early universe to astronomical scales, leaving their imprint in the distribution of light and matter in the universe today. We will also explore the characteristic imprint of Einstein's general relativity and the role of dark energy in shaping the evolution of structure in our Universe. Additionally, our analyses will shed light on the properties of dark matter, which we can "see" via gravity but which does not interact like normal matter. We will also obtain a fuller understanding of the characteristics of galaxies throughout cosmic time. This will tell us whether the usual assumptions about dark matter provide an adequate description of the formation and evolution of galaxies.ICG staff are committed to public outreach and have been engaged in a number of high-profile activities in the media and local community. For example, our staff have visited many local schools to discuss their careers, their research, and share their enthusiasm for astrophysics and cosmology, e.g. BBC Stargazing Live for the last few years with thousands of participants
期刊论文(10)
专著(0)
科研奖励(0)
会议论文
Dark Energy Survey Year 1 Results: Cosmological constraints from cluster abundances and weak lensing
暗能量调查第一年结果:星团丰度和弱透镜效应的宇宙学限制
DOI: 10.1103/physrevd.102.023509
发表时间: 2020
期刊: Physical Review D
影响因子: 5
作者: [Abbott T]
通讯作者: Abbott T
DOI: 10.1088/1748-0221/16/08/p08035
发表时间: 2020-10
期刊: Journal of Instrumentation
影响因子: 1.3
作者: [Q. Abarr;P. Allison;J. Ammerman Yebra;J. Alvarez-Muñiz;J. Beatty;D. Besson;P. Chen;Y. Chen;C. Xie;J. Clem;A. Connolly;L. Cremonesi;C. Deaconu;J. Flaherty;D. Frikken;P. Gorham;C. Hast;C. Hornhuber;J. Huang;K. Hughes;A. Hynous;Y. Ku;C. Kuo;T. Liu;Z. Martin;C. Miki;J. Nam;R. Nichol;K. Nishimura;A. Novikov;A. Nozdrina;E. Oberla;S. Prohira;R. Prechelt;B. Rauch;J. M. Roberts;A. Romero-Wolf;J. W. Russell;D. Seckel;J. Shiao;D. Smith;D. Southall;G. Varner;A. Vieregg;S. Wang;Y. Wang;S. Wissel;R. Young;E. Zas;A. Zeolla]
通讯作者: Q. Abarr;P. Allison;J. Ammerman Yebra;J. Alvarez-Muñiz;J. Beatty;D. Besson;P. Chen;Y. Chen;C. Xie;J. Clem;A. Connolly;L. Cremonesi;C. Deaconu;J. Flaherty;D. Frikken;P. Gorham;C. Hast;C. Hornhuber;J. Huang;K. Hughes;A. Hynous;Y. Ku;C. Kuo;T. Liu;Z. Martin;C. Miki;J. Nam;R. Nichol;K. Nishimura;A. Novikov;A. Nozdrina;E. Oberla;S. Prohira;R. Prechelt;B. Rauch;J. M. Roberts;A. Romero-Wolf;J. W. Russell;D. Seckel;J. Shiao;D. Smith;D. Southall;G. Varner;A. Vieregg;S. Wang;Y. Wang;S. Wissel;R. Young;E. Zas;A. Zeolla
DOI: 10.1103/physrevd.94.022001
发表时间: 2015-07
期刊: Physical Review D
影响因子: 5
作者: [The Dark Energy Survey Collaboration;T. Abbott;F. Abdalla;S. Allam;A. Amara;J. Annis;R. Armstrong;D. Bacon;M. Banerji;A. Bauer;E. Baxter;M. Becker;A. Benoit-Lévy;R. Bernstein;G. Bernstein;E. Bertin;J. Blazek;C. Bonnett;S. Bridle;D. Brooks;C. Bruderer;E. Buckley-Geer;D. Burke;M. Busha;D. Capozzi;A. Rosell;M. Kind;J. Carretero;F. Castander;C. Chang;J. Clampitt;M. Crocce;C. Cunha;C. D'Andrea;L. Costa;R. Das;D. Depoy;S. Desai;H. Diehl;J. Dietrich;S. Dodelson;P. Doel;A. Drlica-Wagner;G. Efstathiou;T. Eifler;B. Erickson;J. Estrada;A. Evrard;A. F. Neto;E. Fernandez;D. Finley;B. Flaugher;P. Fosalba;O. Friedrich;J. Frieman;C. Gangkofner;J. García-Bellido;E. Gaztañaga;D. Gerdes;D. Gruen;R. Gruendl;G. Gutiérrez;W. Hartley;M. Hirsch;K. Honscheid;E. Huff;B. Jain;D. James;M. Jarvis;T. Kacprzak;S. Kent;D. Kirk;E. Krause;A. Kravtsov;K. Kuehn;N. Kuropatkin;J. Kwan;O. Lahav;B. Leistedt;T. Li;M. Lima;H. Lin;N. MacCrann;M. March;J. Marshall;P. Martini;R. McMahon;Peter Melchior;C. Miller;R. Miquel;J. Mohr;E. Neilsen;R. Nichol;A. Nicola;B. Nord;R. Ogando;A. Palmese;H. Peiris;A. Plazas;A. Réfrégier;N. Roe;A. Romer;A. Roodman;B. Rowe;E. Rykoff;C. Sabiu;I. Sadeh;M. Sako;S. Samuroff;C. S'anchez;E. Sánchez;H. Seo;I. Sevilla-Noarbe;E. Sheldon;R. C. Smith;M. Soares-Santos;F. Sobreira;E. Suchyta;M. Swanson;G. Tarlé;J. Thaler;D. Thomas;M. Troxel;V. Vikram;A. Walker;R. Wechsler;J. Weller;Y. Zhang;J. Zuntz]
通讯作者: The Dark Energy Survey Collaboration;T. Abbott;F. Abdalla;S. Allam;A. Amara;J. Annis;R. Armstrong;D. Bacon;M. Banerji;A. Bauer;E. Baxter;M. Becker;A. Benoit-Lévy;R. Bernstein;G. Bernstein;E. Bertin;J. Blazek;C. Bonnett;S. Bridle;D. Brooks;C. Bruderer;E. Buckley-Geer;D. Burke;M. Busha;D. Capozzi;A. Rosell;M. Kind;J. Carretero;F. Castander;C. Chang;J. Clampitt;M. Crocce;C. Cunha;C. D'Andrea;L. Costa;R. Das;D. Depoy;S. Desai;H. Diehl;J. Dietrich;S. Dodelson;P. Doel;A. Drlica-Wagner;G. Efstathiou;T. Eifler;B. Erickson;J. Estrada;A. Evrard;A. F. Neto;E. Fernandez;D. Finley;B. Flaugher;P. Fosalba;O. Friedrich;J. Frieman;C. Gangkofner;J. García-Bellido;E. Gaztañaga;D. Gerdes;D. Gruen;R. Gruendl;G. Gutiérrez;W. Hartley;M. Hirsch;K. Honscheid;E. Huff;B. Jain;D. James;M. Jarvis;T. Kacprzak;S. Kent;D. Kirk;E. Krause;A. Kravtsov;K. Kuehn;N. Kuropatkin;J. Kwan;O. Lahav;B. Leistedt;T. Li;M. Lima;H. Lin;N. MacCrann;M. March;J. Marshall;P. Martini;R. McMahon;Peter Melchior;C. Miller;R. Miquel;J. Mohr;E. Neilsen;R. Nichol;A. Nicola;B. Nord;R. Ogando;A. Palmese;H. Peiris;A. Plazas;A. Réfrégier;N. Roe;A. Romer;A. Roodman;B. Rowe;E. Rykoff;C. Sabiu;I. Sadeh;M. Sako;S. Samuroff;C. S'anchez;E. Sánchez;H. Seo;I. Sevilla-Noarbe;E. Sheldon;R. C. Smith;M. Soares-Santos;F. Sobreira;E. Suchyta;M. Swanson;G. Tarlé;J. Thaler;D. Thomas;M. Troxel;V. Vikram;A. Walker;R. Wechsler;J. Weller;Y. Zhang;J. Zuntz
DOI: 10.1103/physrevd.98.043526
发表时间: 2017-08
期刊: Physical Review D
影响因子: 5
作者: [T. Abbott;F. Abdalla;A. Alarcon;J. Aleksić;S. Allam;S. Allen;A. Amara;J. Annis;J. Asorey-J.-As]
通讯作者: T. Abbott;F. Abdalla;A. Alarcon;J. Aleksić;S. Allam;S. Allen;A. Amara;J. Annis;J. Asorey-J.-As
10
    Core Equipment Award 2022
    • 批准号:
      EP/X034933/1
    • 项目类别:
      Research Grant
    • 资助金额:
      $110.86万
    • 财政年份:
      2023
    • 负责人:
      Robert Nichol
    • 依托单位:
    Developing synergies between transient astronomy and early medical intervention
    • 批准号:
      ST/S002308/1
    • 项目类别:
      Research Grant
    • 资助金额:
      $9.08万
    • 财政年份:
      2018
    • 负责人:
      Robert Nichol
    • 依托单位:
    SEPNet IPS Fellowship (Main host proposal from Portsmouth)
    • 批准号:
      ST/M000206/1
    • 项目类别:
      Fellowship
    • 资助金额:
      $11.64万
    • 财政年份:
      2015
    • 负责人:
      Robert Nichol
    • 依托单位:
    DESI: The Dark Energy Spectroscopic Instrument
    • 批准号:
      ST/M002853/1
    • 项目类别:
      Research Grant
    • 资助金额:
      $4.67万
    • 财政年份:
      2015
    • 负责人:
      Robert Nichol
    • 依托单位:
    国内基金
    海外基金
    中英“天体物理(astrophysics)”领域双边研讨会
    • 批准号:
      11921003
    • 项目类别:
      国际(地区)合作与交流项目
    • 资助金额:
      1.5万元
    • 批准年份:
      2019
    • 负责人:
      常进
    • 依托单位:
    中英“天体物理(astrophysics)”领域双边研讨会
    • 批准号:
      11927804
    • 项目类别:
      国际(地区)合作与交流项目
    • 资助金额:
      1.4万元
    • 批准年份:
      2019
    • 负责人:
      吴学兵
    • 依托单位:
    中英“天体物理(astrophysics)”领域双边研讨会
    • 批准号:
      11981230269
    • 项目类别:
      国际(地区)合作与交流项目
    • 资助金额:
      1.5万元
    • 批准年份:
      2019
    • 负责人:
      高亮
    • 依托单位:
    中英“天体物理(astrophysics)”领域双边研讨会
    • 批准号:
      --
    • 项目类别:
      --
    • 资助金额:
      1.8万元
    • 批准年份:
      2019
    • 负责人:
      林隽
    • 依托单位: