Cosmology Rolling Grant: Case for Renewal

宇宙学滚动资助：续签的理由

• 批准号: ST/G000549/1
• 负责人: John McDonald
• 金额: $ 15.75万
• 依托单位: Lancaster University
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2008
• 资助国家: 英国
• 起止时间: 2008 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FG000549%2F1
• 关键词: Cosmology; Rolling; Grant; Case; Renewal

In 2008 the world's most powerful probe of fundamental physics, the Large Hadron Collider (LHC) particle accelerator at CERN, will begin operation. In the same year the European Space Agency will launch the Planck satellite observatory, which will observe the Cosmic Microwave Background (CMB) in unprecedented detail. From these two experimental programmes there is the exciting prospect of epoch-making breakthroughs in our understanding of the fundamental theory of particles and forces and of the 'seed' density perturbations from which galaxies and larger cosmological structures grow. The fusion of these new discoveries could shed light on the identity of dark matter, which constitutes 25% of the matter in the Universe, the mystery of the gravity-repelling 'dark energy' which makes up 70% of the Universe, the origin of the matter-antimatter asymmetry (why the Universe is made of protons and not anti-protons) and the nature of the very earliest epoch in the history of the Universe, known as Inflation, during which the seed perturbations for galaxy formation are created. Particle cosmology, as it is known, directly addresses these fundamental questions from the point of view of theoretical particle physics. Its primary goal is to construct a consistent history of the Universe from its earliest epoch. Particle cosmology also provides a testing ground for new particle physics theories, using the hot Big Bang as an extremely powerful particle accelerator from which important constraints on new theories can be deduced. The ambitious five year research programme of the proposal will seek to exploit the new discoveries from LHC and Planck to gain deep insights into the history of the Universe. The programme will address all the major themes in modern particle cosmology. Objectives of the programme include: the nature of dark matter; the connection between Inflation and LHC experiments; the development of particle theories of Inflation and the origin of galaxy seeds; the study of unconventional 'non-Gaussian' signatures in the cosmic microwave background; the origin of magnetic fields of the size of a galaxy, which may originate during the Inflation era; the connection between string theory and dark energy. Through insights gained from particle cosmology, the programme will seek to suggest new experimental targets for LHC experiments and new features in the CMB to be studied by Planck.

2008年，世界上最强大的基础物理探测器，欧洲核子研究中心的大型强子对撞机（LHC）粒子加速器，将开始运行。同年，欧洲航天局将发射普朗克卫星天文台，它将以前所未有的细节观测宇宙微波背景（CMB）。从这两个实验项目中，我们可以看到令人兴奋的前景，即在我们对粒子和力的基本理论以及星系和更大的宇宙学结构从中生长出来的“种子”密度扰动的理解方面，有划时代的突破。这些新发现的融合可以揭示暗物质的身份，它构成了宇宙中25%的物质，构成宇宙70%的重力排斥“暗能量”的奥秘，物质-反物质不对称的起源（为什么宇宙是由质子而不是反质子组成的）和宇宙历史上最早的时代的性质，被称为通货膨胀，在此期间，星系形成的种子扰动被创造出来。众所周知，粒子宇宙学直接从理论粒子物理学的角度来解决这些基本问题。它的主要目标是从最早的时代开始构建一个一致的宇宙历史。粒子宇宙学也为新的粒子物理学理论提供了一个试验场，使用热大爆炸作为一个非常强大的粒子加速器，从中可以推导出对新理论的重要约束。该计划雄心勃勃的五年研究计划将寻求利用LHC和普朗克的新发现，以深入了解宇宙的历史。该方案将涉及现代粒子宇宙学的所有主要主题。该计划的目标包括：暗物质的本质;暴胀与大型强子对撞机实验之间的联系;暴胀粒子理论的发展和星系种子的起源;研究宇宙微波背景中的非常规“非高斯”特征;星系大小的磁场的起源，可能起源于暴胀时代;弦理论与暗能量之间的联系。通过从粒子宇宙学中获得的见解，该方案将寻求为LHC实验提出新的实验目标，并为普朗克研究的CMB提出新的特征。

项目成果

Cosmic ray anomalies and dark matter annihilation to muons via a Higgs portal hidden sector

• DOI: 10.1103/physrevd.81.023530
• 发表时间: 2009-05
• 期刊: Physical Review D
• 影响因子: 5
• 作者: K. Kohri;J. McDonald;N. Sahu

Vector Curvaton without Instabilities

无不稳定性的矢量曲率

• DOI: 10.48550/arxiv.0909.0475
• 发表时间: 2009
• 作者: Dimopoulos K

Vector Curvaton with varying Kinetic Function

具有不同动力学函数的矢量曲率

• DOI: 10.48550/arxiv.0907.1838
• 发表时间: 2009
• 作者: Dimopoulos K

Cosmological evolution of scalar fields and gravitino dark matter in gauge mediation at low reheating temperatures

低再加热温度下规范介导中标量场和引力暗物质的宇宙学演化

• DOI: 10.1088/1475-7516/2010/02/003
• 发表时间: 2010
• 期刊: Journal of Cosmology and Astroparticle Physics
• 影响因子: 6.4
• 作者: Ferrantelli A

Enhanced dark matter annihilation rate for positron and electron excesses from Q-ball decay.

增强 Q 球衰变导致的正电子和电子过量的暗物质湮灭率。

• DOI: 10.1103/physrevlett.103.151301
• 发表时间: 2009
• 期刊: Physical review letters
• 影响因子: 8.6
• 作者: McDonald J