Fundamental physics from the large-scale structure of the Universe
Fundamental physics from the large-scale structure of the Universe
批准号:
ST/W004755/1
负责人:
Eva-Maria Mueller
金额:
$67.39万
依托单位:
依托单位国家:
英国
项目类别:
Fellowship
财政年份:
2023
资助国家:
英国
项目状态:
未结题
起止时间:
2023 至 --
中文摘要
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英文摘要
What happened in the first second after the Big Bang? Why is the expansion of the Universe accelerating? And what is dark energy?Our Universe still holds many mysteries, from its earliest beginnings to its current accelerated expansion. While studying the origin and evolution of our Universe is exciting by itself, what especially drives me is the link of cosmology to fundamental physical theories. The Universe is the largest laboratory we have to push our understanding of the laws of physics!While the physics of the early Universe and the underlying cause of dark energy remains puzzling, what is certain is that we can study both through the clustering of galaxies in our Universe. My research focuses on analysing the large scale structure of galaxies in our Universe to uncover the underlying nature of dark energy and determine the physical theory that drives the expansion of the Universe milli-seconds after the Big Bang.The Dark Energy Spectroscopic Instrument (DESI) is designed to tackle these questions: after more than a decade of development, DESI achieved first light in 2019. This year DESI began its 5-year survey mapping the 3D positions of tens of millions of galaxies across almost half the sky. I joined DESI during my PhD and am excited to see the project evolve from being a mere proposal to finally start my research with its first year of data that will have pivotal impact on cosmology and our understanding of fundamental physics.
期刊论文(2)
专著(0)
科研奖励(0)
会议论文
Optimal 1D Ly a forest power spectrum estimation - III. DESI early data
最优一维 Ly 森林功率谱估计 - III。
DOI:
10.1093/mnras/stae171
发表时间:
2024
期刊:
Monthly Notices of the Royal Astronomical Society
影响因子:
4.8
作者:
[Karaçayli N]
通讯作者:
Karaçayli N
Measurement of the matter-radiation equality scale using the extended baryon oscillation spectroscopic survey quasar sample
使用扩展重子振荡光谱测量类星体样本测量物质-辐射相等尺度
DOI:
10.1093/mnras/stad1867
发表时间:
2023
期刊:
Monthly Notices of the Royal Astronomical Society
影响因子:
4.8
作者:
[Bahr-Kalus B]
通讯作者:
Bahr-Kalus B
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