课题基金 / 基金详情

Physics and Cosmology with Supernovae

Physics and Cosmology with Supernovae
超新星的物理学和宇宙学
批准号:
ST/L000679/1
负责人:
Mark Sullivan
金额:
$20.32万
依托单位:
依托单位国家:
英国
项目类别:
Research Grant
财政年份:
2014
资助国家:
英国
项目状态:
已结题
起止时间:
2014 至 --

项目摘要

项目成果

Mark Sullivan的其他基金

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中文摘要
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英文摘要
The quest to understand what the universe is made of has fired our imagination for thousands of years. Finding the answer has inspired the creativity of generations of scientists, so it may come as a surprise that the nature of over 90% of the Universe is a mystery to us. We know that most of the matter in the Universe is invisible to us, in an unknown form called "dark matter". We also know that the Universe is getting bigger, an expansion driven by a "Big Bang" nearly 14 billion years ago. As the Universe contains objects like stars and planets as well as the unseen dark matter, gravity pulling everything together should slow down this expansion. However, experiments in the last 15 years have come to a quite different conclusion: Our Universe is expanding at an ever faster speed -- the opposite to the effect of gravity.This presents one of the most exciting challenges to modern science: the quest to understand this unexpected acceleration. The unknown substance responsible is called "dark energy"; as the name suggests we know little about it. We think that it makes up about 70% of the Universe with an incredibly low density -- much less than a speck of dust in a volume of space the size of the Earth. Beyond that, there are only theories; perhaps most shockingly, some believe that Einstein's theory of general relativity, the bedrock of modern cosmology, simply doesn't work on the largest scales.This project lays the foundation to test these theories using cosmic explosions known as supernovae, violent thermonuclear explosions from dying stars that can outshine entire galaxies. These supernovae always explode with about the same brightness, and are "standard candles" or cosmic rulers which can measure vast intergalactic distances. I hunt out these supernovae billions of light-years away, and measure their brightness as they appear to us on Earth. When combined with a knowledge of their intrinsic brightness we can infer their distance, and, from that, information about the mysterious dark energy.Recent research has unexpectedly thrown up a extraordinary variety of new types of these supernova explosions. New surveys, charting huge areas of the sky on unprecedented short time-scales, are finding cosmic explosions for which we have no explanation -- from ultra-luminous supernova explosions seen almost to the edge of the universe, to faint blips that barely register on our detectors. Not only is understanding dark energy a challenge, but these new explosion types suggest that the tools that we use for its study may also be poorly understood. This project will investigate the physics of the standard candles that we take for granted.Though this project has limited practical application, there are fewer more fundamental questions about Nature that remain to be answered than the question of dark energy. Understanding the Universe we live in has challenged us ever since early humans became fascinated by the environment around them. Research such as this continues our exploration and understanding of the Universe that surrounds and intrigues us.
期刊论文(10)
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科研奖励(0)
会议论文
DOI: 10.1093/mnras/stv1888
发表时间: 2015-01
期刊: Monthly Notices of the Royal Astronomical Society
影响因子: 4.8
作者: [M. Graham;P. Nugent;M. Sullivan;A. Filippenko;S. Cenko;J. Silverman;K. Clubb;W. Zheng]
通讯作者: M. Graham;P. Nugent;M. Sullivan;A. Filippenko;S. Cenko;J. Silverman;K. Clubb;W. Zheng
DOI: 10.1093/mnras/stv106
发表时间: 2014-10
期刊: Monthly Notices of the Royal Astronomical Society
影响因子: 4.8
作者: [C. Barbarino;M. Dall’ora;M. Botticella;M. Valle;L. Zampieri;J. Maund;M. L. Pumo;A. Jerkstrand;S. Benetti;N. Elias-Rosa;M. Fraser;A. Gal-yam;M. Hamuy;M. Hamuy;C. Inserra;C. Knapic;A. Lacluyze;M. Molinaro;P. Ochner;A. Pastorello;G. Pignata;D. Reichart;C. Ries;A. Riffeser;B. Schmidt;M. Schmidt;R. Smareglia;S. Smartt;K. Smith;J. Sollerman;M. Sullivan;L. Tomasella;M. Turatto;S. Valenti;O. Yaron;D. Young]
通讯作者: C. Barbarino;M. Dall’ora;M. Botticella;M. Valle;L. Zampieri;J. Maund;M. L. Pumo;A. Jerkstrand;S. Benetti;N. Elias-Rosa;M. Fraser;A. Gal-yam;M. Hamuy;M. Hamuy;C. Inserra;C. Knapic;A. Lacluyze;M. Molinaro;P. Ochner;A. Pastorello;G. Pignata;D. Reichart;C. Ries;A. Riffeser;B. Schmidt;M. Schmidt;R. Smareglia;S. Smartt;K. Smith;J. Sollerman;M. Sullivan;L. Tomasella;M. Turatto;S. Valenti;O. Yaron;D. Young
DOI: 10.1093/mnras/stv1919
发表时间: 2015-02
期刊: Monthly Notices of the Royal Astronomical Society
影响因子: 4.8
作者: [M. Fraser;R. Kotak;A. Pastorello;A. Jerkstrand;S. Smartt;Ting-Wan Chen;M. Childress;G. Gilmore]
通讯作者: M. Fraser;R. Kotak;A. Pastorello;A. Jerkstrand;S. Smartt;Ting-Wan Chen;M. Childress;G. Gilmore
DOI: 10.1088/2041-8205/799/1/l2
发表时间: 2014-10
期刊: The Astrophysical Journal Letters
影响因子: --
作者: [C. Inserra;S. Sim;L. Wyrzykowski;L. Wyrzykowski;S. Smartt;M. Fraser;M. Nicholl;K. Shen;A. Jerkstrand;A. Gal-yam;D. Howell;D. Howell;K. Maguire;P. Mazzali;S. Valenti;S. Valenti;S. Taubenberger;S. Benitez-Herrera;D. Bersier;N. Blagorodnova;H. Campbell;Ting-Wan Chen;N. Elias-Rosa;W. Hillebrandt;Z. Kostrzewa-Rutkowska;S. Kozłowski;M. Kromer;J. Lyman;J. Polshaw;F. Röpke;A. Ruiter;K. Smith;S. Spiro;M. Sullivan;O. Yaron;D. Young;F. Yuan]
通讯作者: C. Inserra;S. Sim;L. Wyrzykowski;L. Wyrzykowski;S. Smartt;M. Fraser;M. Nicholl;K. Shen;A. Jerkstrand;A. Gal-yam;D. Howell;D. Howell;K. Maguire;P. Mazzali;S. Valenti;S. Valenti;S. Taubenberger;S. Benitez-Herrera;D. Bersier;N. Blagorodnova;H. Campbell;Ting-Wan Chen;N. Elias-Rosa;W. Hillebrandt;Z. Kostrzewa-Rutkowska;S. Kozłowski;M. Kromer;J. Lyman;J. Polshaw;F. Röpke;A. Ruiter;K. Smith;S. Spiro;M. Sullivan;O. Yaron;D. Young;F. Yuan
10
    STFC IAA Southampton
    • 批准号:
      ST/X508184/1
    • 项目类别:
      Research Grant
    • 资助金额:
      $19.11万
    • 财政年份:
      2022
    • 负责人:
      Mark Sullivan
    • 依托单位:
    STFC Innovations Partnership Scheme Fellow at the University of Southampton
    • 批准号:
      ST/W000393/1
    • 项目类别:
      Fellowship
    • 资助金额:
      $41.44万
    • 财政年份:
      2021
    • 负责人:
      Mark Sullivan
    • 依托单位:
    Support for telescope travel for Southampton Astronomy research group
    • 批准号:
      ST/N001540/1
    • 项目类别:
      Research Grant
    • 资助金额:
      $2.06万
    • 财政年份:
      2015
    • 负责人:
      Mark Sullivan
    • 依托单位:
    UK Involvement in LSST: Phase A
    • 批准号:
      ST/N002504/1
    • 项目类别:
      Research Grant
    • 资助金额:
      $22.73万
    • 财政年份:
      2015
    • 负责人:
      Mark Sullivan
    • 依托单位:
    海外基金