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

String Theory and Quantum Field Theory: From the Planck Scale to the Hubble Scale

弦理论和量子场论：从普朗克尺度到哈勃尺度

基本信息

批准号：
2210562
负责人：
Willy Fischler
金额：
$ 102万
依托单位：
University of Texas at Austin
依托单位国家：
美国
项目类别：
Continuing Grant
财政年份：
2022
资助国家：
美国
起止时间：
2022-08-01 至 2025-07-31
项目状态：
未结题

来源：
https://www.nsf.gov/awardsearch/showAward?AWD_ID=2210562&HistoricalAwards=false
关键词：
String Theory Quantum Field Planck

项目摘要

This award funds the research activities of Professors Elena Cáceres, Jacques Distler, Willy Fischler, Can Kilic, and Sonia Paban at the University of Texas at Austin.The research of Professors Cáceres, Distler, Fischler, Kilic, and Paban is focused on discovering and understanding the laws that govern the universe at the most fundamental level. This research utilizes diverse and multi-pronged approaches to achieving this mission. These include studying the extensions to the so-called Standard Model, which governs the behavior of the elementary particles, and the associated experimental signatures of such extensions. These also include the study of early-universe cosmology and present-day astrophysics, and exploring the physics of black holes, which may shed light on how a quantum theory of gravity may be formulated. Finally, this research also includes studies in relativistic quantum field theory (the mathematical language in which theories of the elementary particles are expressed) and string theory (which aims to unify all of the different particles and forces in nature). Since the early days of modern physics, the United States has led the effort in the discovery of these fundamental laws. Therefore, more research in this direction is in the national interest, and Professors Cáceres, Distler, Fischler, Kilic, and Paban are committed to making further research contributions in these directions. In addition, this research will involve graduate students and postdoctoral researchers and provide scientific training that should serve these junior scientists well throughout their careers both within and outside academia. Finally, these professors make science outreach a priority. They regularly deliver public lectures, organize activities to increase science literacy, and foster the participation of underrepresented minorities in physics.More specifically, many different research areas are to be investigated as part of this research project. Professor Cáceres will continue her work on quantum models that are holographic duals of black holes. In particular, she will focus on observables that inform us about the wormhole interior. Professor Distler will continue his exploration of 4D N=2 superconformal field theories and their properties. He will expand on his investigations of continuum QFTs exhibiting fractonic behavior and he will study new defects in string theory. Professor Fischler will continue to work with his students on quantum information in quantum gravity (using gauge-gravity duality) and the use of the quantum Hall effect in the context of quantum computation. He will continue to work on holographic spacetime and in particular the quantum mechanics of de Sitter spacetime which he helped to pioneer twenty years ago. This is particularly timely in light of renewed interest on the nature of quantum de Sitter space-time. Professor Kilic will explore the experimental signatures of new particles that couple to the Standard Model through minimal interactions, called 'portals'. He will also apply machine-learning techniques to extend the reach of searches at the Large Hadron Collider to new physics scenarios that are challenging to discover. He will study models of dark matter that can help address discrepancies in existing measurements of cosmological parameters. Professor Paban's work will focus on new cosmic inflation models in light of new insights from string theory and the stabilization of internal moduli. Particular emphasis will be placed on the production of gravitational waves and primordial black holes in these inflation models.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

该奖项资助了位于奥斯汀的德克萨斯大学的Elena Cáceres、Jacques Distler、Willy Fischler、Can Kilic和Sonia Paban教授的研究活动。Cáceres、Distler、Fischler、Kilic和Paban教授的研究重点是发现和理解在最基本的层面上支配宇宙的定律。这项研究采用了多种多样、多管齐下的方法来实现这一使命。其中包括研究所谓的标准模型的扩展，标准模型控制基本粒子的行为，以及这种扩展的相关实验特征。这些还包括对早期宇宙宇宙学和当今天体物理学的研究，以及对黑洞物理学的探索，这可能会为如何制定量子引力理论提供启示。最后，这项研究还包括相对论量子场论（表达基本粒子理论的数学语言）和弦理论（旨在统一自然界中所有不同的粒子和力）的研究。从现代物理学的早期开始，美国就在发现这些基本定律的努力中处于领先地位。因此，在这个方向上进行更多的研究符合国家利益，Cáceres、Distler、Fischler、Kilic和Paban教授致力于在这些方向上做出进一步的研究贡献。此外，这项研究将涉及研究生和博士后研究人员，并提供科学培训，为这些初级科学家在学术界内外的职业生涯提供良好的服务。最后，这些教授把科学推广作为首要任务。他们定期发表公开演讲，组织活动以提高科学素养，并促进未被充分代表的少数民族参与物理学。更具体地说，作为这个研究项目的一部分，许多不同的研究领域将被调查。Cáceres教授将继续研究量子模型，即黑洞的全息对偶。特别是，她将专注于告诉我们关于虫洞内部的可观察到的东西。Distler教授将继续探索4D N=2超共形场理论及其性质。他将扩展他对表现分形行为的连续qft的研究，并将研究弦理论中的新缺陷。Fischler教授将继续与他的学生一起研究量子引力中的量子信息（使用量规引力对偶）以及在量子计算背景下使用量子霍尔效应。他将继续研究全息时空，特别是他在20年前帮助开创的德西特时空的量子力学。鉴于人们对量子德西特时空的性质重新产生了兴趣，这是特别及时的。Kilic教授将探索新粒子的实验特征，这些新粒子通过最小的相互作用与标准模型耦合，称为“门户”。他还将应用机器学习技术，将大型强子对撞机的搜索范围扩展到具有挑战性的新物理场景。他将研究暗物质模型，以帮助解决现有宇宙参数测量中的差异。帕潘教授的工作将集中在新的宇宙膨胀模型上，根据弦理论的新见解和内模的稳定。在这些暴胀模型中，将特别强调引力波和原始黑洞的产生。该奖项反映了美国国家科学基金会的法定使命，并通过使用基金会的知识价值和更广泛的影响审查标准进行评估，被认为值得支持。