权益分类	功能权益	普通用户	{{item.name}}会员
{{category.name}}	{{benefitItem.name}}

University of Sussex Astronomy Consolidated Grant 2023-2026

苏塞克斯大学天文学综合补助金 2023-2026

基本信息

批准号：
ST/X001040/1
负责人：
Stephen Wilkins
金额：
$ 368.13万
依托单位：
University of Sussex
依托单位国家：
英国
项目类别：
Research Grant
财政年份：
2023
资助国家：
英国
起止时间：
2023 至无数据
项目状态：
未结题

来源：
https://gtr.ukri.org/projects?ref=ST%2FX001040%2F1
关键词：
University Sussex Astronomy Consolidated Grant

项目摘要

This proposal seeks support to continue an extensive programme of research into extragalactic astrophysics and cosmology, by addressing some of the most pressing astrophysical questions of our time, such as:- What are the laws of physics operating in the early Universe?- How did the initial structure in the universe form?- How is the universe evolving and what roles do dark matter and dark energy play?- When and how were the first stars, black holes and galaxies born?- How do stars and galaxies evolve?To achieve these aims we will combine cutting-edge observations, numerical simulations, and statistical techniques. This proposal consists of 10 varied but interconnected projects, each involving one or more faculty members and researchers, that can be collected into three broad themes: Early and late universe cosmology; Galaxy simulation and modelling; Galaxy and cluster observations and analysis:Early and late universe cosmology: a series of projects will address theoretical predictions and observational constraints on inflation, dark energy and large scale structure. Our work encompasses both the development of theoretical frameworks and the analysis of cutting edge observational data-sets.Galaxy simulation and modelling: we will use Peta-scale computing facilities to carry out detailed studies of the formation and evolution of the first structures, and make statistical predictions that can be used in the exploitation of current and upcoming observational facilities such as James Webb Space Telescope, Euclid, LOFAR, and the Square Kilometre Array.Galaxy and cluster observations: we will make use of multi-wavelength observations to answer a variety of questions concerning the formation and evolution of galaxies. We will continue to exploit our involvement in the Dark Energy Survey, Euclid, the James Webb Space Telescope, the 4m Multi-Object Spectroscopic Telescope (4MOST) on VISTA, LOFAR, the Vera Rubin Observatory, and the XMM-Newton Cluster Survey. We also request support for an outreach project attached to Project 10.

这项建议寻求支持，以继续对河外天体物理学和宇宙学进行广泛的研究，解决我们时代一些最紧迫的天体物理学问题，例如：宇宙的初始结构是如何形成的？宇宙是如何演化的，暗物质和暗能量扮演着什么角色？第一批恒星、黑洞和星系是何时以及如何诞生的？恒星和星系是如何演化的？为了实现这些目标，我们将结合联合收割机尖端的观察，数值模拟和统计技术。该提案由10个不同但相互关联的项目组成，每个项目涉及一名或多名教职员工和研究人员，可以收集到三个广泛的主题：早期和晚期宇宙学;星系模拟和建模;星系和星系团观测和分析：早期和晚期宇宙学：一系列项目将解决理论预测和观测约束膨胀，暗能量和大尺度结构。我们的工作包括理论框架的发展和尖端观测数据集的分析。星系模拟和建模：我们将使用千万亿次计算设备对第一批结构的形成和演化进行详细的研究，并进行统计预测，这些预测可以用于利用现有的和即将到来的观测设备，如詹姆斯·韦伯太空望远镜、欧几里得、LOFAR、星系和星系团观测：我们将利用多波长观测来回答有关星系形成和演化的各种问题。我们将继续利用我们参与的暗能量调查，欧几里得，詹姆斯韦伯太空望远镜，VISTA上的4米多目标光谱望远镜（4 MOST），LOFAR，Vera Rubin天文台和XMM-牛顿星系团调查。我们还请求支持项目10所附的一个外联项目。