1,721,181 research outputs found

    Quantum Gravity and Predictions for our Universe

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    In this talk I provide an executive summary of some of the recent progress that has been made in understanding some key features of quantum gravitational theories.  This is rooted in lessons learned from the landscape of consistent solutions to string theory and captured by the principles of the Swampland program.   A key feature of this is the lack of decoupling between short and long distance descriptions of the theory leading to a radical revision of the notion of consistency of effective field theories.  This opens up a new window into unresolved fine tuning  problems for particle physics and cosmology.   I will further explain how these ideas lead to concrete experimentally verifiable predictions for our universe. Cumrun Vafa Cumrun Vafa is the Hollis Professor of Mathematicks and Natural Philosophy in the Physics Department at Harvard University, where he does research and teaches theoretical physics since 1985.  Born in Iran in 1960, he moved to the US for higher education where he received his B.S. in math and physics from MIT before moving to Princeton University, where he received his Ph.D. in theoretical physics. Coffee and tea served at 16:00pm</p

    G(2) holonomy, Taubes' construction of Seiberg-Witten invariants and superconducting vortices

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    Using a reformulation of topological N = 2 QFT’s in M-theory setup, where QFT is realized via M5 branes wrapping co-associative cycles in a G2 manifold constructed from the space of self-dual 2-forms over a four-fold X, we show that superconducting vortices are mapped to M2 branes stretched between M5 branes. This setup provides a physical explanation of Taubes’ construction of the Seiberg-Witten invariants when X is symplectic and the superconducting vortices are realized as pseudo-holomorphic curves. This setup is general enough to realize topological QFT’s arising from N = 2 QFT’s from all Gaiotto theories on arbitrary 4-manifolds. © 2020, The Author(s)

    Ray-Singer Torsion, Topological Strings and Black Holes

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    Genus one amplitude for topological strings on Calabi-Yau 3-folds can be computed using mirror symmetry: The partition function at genus one gets mapped to a holomorphic version of Ray-Singer torsion on the mirror Calabi-Yau. On the other hand it can be shown by a physical argument that this gives a curvature squared correction term to the gravitational action. This in paticular leads to an effective quantum gravity cutoff known as the species scale, which varies over moduli space of Calabi-Yau manifolds. This resolves some of the puzzles associated to the entropy of small black holes when there are a large number of light species of particles. Thus Ray-Singer torsion, via its connection to topological strings at genus one, provides a measure of light degrees of freedom of four dimensional N=2 supergravity theories. Based on a talk given on May 12th, 2023 at the Singer Memorial Conference, MIT.Comment: 11 page

    String Phenomenology 2019

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    I present some recent progress in formulating new swampland criteria
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