物理学科Seminar第757讲 双场理论下的O(D,D)弦宇宙学

创建时间:  2025/09/22  邵奋芬   浏览次数:   返回

报告题目 (Title):O(D,D) string cosmology from double field theory

(双场理论下的O(D,D)弦宇宙学)

报告人 (Speaker):Dr. Stephen Angus(韩国西江大学)

报告时间 (Time):2025年9月24日(周三) 10:00-11:40

报告地点 (Place):校本部 AJ204

邀请人 (Inviter):尹璐

主办部门:理学院物理系

摘要 (Abstract):

The low-energy limit of string theory contains additional gravitational degrees of freedom that are not present in general relativity. Together with the metric, these fields are naturally embedded in the O(D,D)-symmetric framework of double field theory (DFT). First I will explain how the O(D,D) symmetry uniquely prescribes the interactions between the extended gravitational sector and other matter, leading to novel features beyond conventional string cosmology. Then I will present the equations of motion for linear perturbations, and I will show how the generalized conservation laws modify the conditions for conservation of curvature perturbations. Finally, I will present some examples of analytic solutions, including candidate models for bouncing cosmologies, and I will explore how they may imply a non-Riemannian origin of the universe.

上一条:物理学科Seminar第758讲 非对易时空的宇宙微波背景辐射限制

下一条:数学学科Seminar第2902讲 非线性模型降阶及其应用


物理学科Seminar第757讲 双场理论下的O(D,D)弦宇宙学

创建时间:  2025/09/22  邵奋芬   浏览次数:   返回

报告题目 (Title):O(D,D) string cosmology from double field theory

(双场理论下的O(D,D)弦宇宙学)

报告人 (Speaker):Dr. Stephen Angus(韩国西江大学)

报告时间 (Time):2025年9月24日(周三) 10:00-11:40

报告地点 (Place):校本部 AJ204

邀请人 (Inviter):尹璐

主办部门:理学院物理系

摘要 (Abstract):

The low-energy limit of string theory contains additional gravitational degrees of freedom that are not present in general relativity. Together with the metric, these fields are naturally embedded in the O(D,D)-symmetric framework of double field theory (DFT). First I will explain how the O(D,D) symmetry uniquely prescribes the interactions between the extended gravitational sector and other matter, leading to novel features beyond conventional string cosmology. Then I will present the equations of motion for linear perturbations, and I will show how the generalized conservation laws modify the conditions for conservation of curvature perturbations. Finally, I will present some examples of analytic solutions, including candidate models for bouncing cosmologies, and I will explore how they may imply a non-Riemannian origin of the universe.

上一条:物理学科Seminar第758讲 非对易时空的宇宙微波背景辐射限制

下一条:数学学科Seminar第2902讲 非线性模型降阶及其应用