Beyond Lorentzian Geometry
from
Monday, 28 October 2019 (09:30)
to
Tuesday, 29 October 2019 (17:00)
Monday, 28 October 2019
09:30
Welcome and registration
Welcome and registration
09:30 - 10:00
10:00
Oddities in non-relativistic strong gravity
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Dieter Van den Bleeken
Oddities in non-relativistic strong gravity
Dieter Van den Bleeken
10:00 - 10:45
I will review the nonrelativisic, or large c, expansion of general relativity and will argue why dynamic matter that sources strong gravitational fields requires the presence of odd powers in this expansion. I will report on ongoing work constructing the effective non-relativistic theory including these odd terms. A number of other peculiarities of the strong field, nonrelativistic corner of GR will be pointed out.
10:45
Coffee break
Coffee break
10:45 - 11:15
11:15
Non-relativistic String Theory and Branes
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Eric Bergshoeff
Non-relativistic String Theory and Branes
Eric Bergshoeff
11:15 - 12:00
The aim of this talk is to describe what we can learn about basic non-relativistic brane solutions in non-relativistic string theory from non-relativistic T-duality in the same way that relativistic T-duality has been applied in the past to relate different relativistic brane solutions. The first part of the talk will be a review of non-relativistic string theory, the equations of motion of the background fields and the T-duality symmetry. In the he second part of the talk, which will be more speculative, we will discuss how we think that non-relativistic branes fit into the picture.
12:10
Maximally symmetric spacetimes reconsidered
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Stefan Prohazka
Maximally symmetric spacetimes reconsidered
Stefan Prohazka
12:10 - 12:55
Spacetimes, like Minkowski space, are omnipresent in physics. I will introduce a recent classification of spacetimes that generalizes the classification of maximally symmetric lorentzian geometries and includes further physically interesting ones. Among them are galilean, carrollian and aristotelian geometries for which there is renewed interest due to applications in holography. These spacetimes posses infinite dimensional (BMS-like) symmetries which we will also discuss.
13:00
Lunch
Lunch
13:00 - 14:30
14:30
Soft degrees of freedom, Gibbons-Hawking contribution and Casimir effect
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Glenn Barnich
Soft degrees of freedom, Gibbons-Hawking contribution and Casimir effect
Glenn Barnich
14:30 - 15:15
The semiclassical contribution to the partition function is obtained by evaluating the Euclidean action improved through suitable boundary terms. We address the question of which degrees of freedom are responsible for this contribution. A physical toy model for the gravitational problem is a charged vacuum capacitor. For a planar charged vacuum capacitor with perfectly conducting plates, we identify the degrees of freedom that, in the quantum theory, give rise to additional contributions to the standard black body result proportional to the area of the plates. They allow for a microscopic derivation of the thermodynamics of the charged capacitor and contribute to the Casimir effect at finite temperature and thus to the entropy.
15:15
Tea
Tea
15:15 - 15:45
15:45
Renormalization Group Flows of Scalar Galilean Electrodynamics in 2 + 1 Dimensions
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Shira Chapman
Renormalization Group Flows of Scalar Galilean Electrodynamics in 2 + 1 Dimensions
Shira Chapman
15:45 - 16:30
I will discuss the theory of Galilean electrodynamics coupled to a single Schrödinger scalar in 2+1 dimensions. This theory, originally obtained from a null-reduction of relativistic Maxwell's theory coupled to a complex scalar field in 3+1 dimensions, suffers an infinite series of quantum corrections. I will explain how these corrections can be handled systematically using the background field method, leading to a continuous manifold of fixed points where the non-relativistic conformal symmetry is preserved.
Tuesday, 29 October 2019
10:00
Quantum Critical and Supersymmetric Lifshitz Field Theories
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Igal Arav
Quantum Critical and Supersymmetric Lifshitz Field Theories
Igal Arav
10:00 - 10:45
I will discuss non-boost-invariant field theories with "time domain" supersymmetry, in which the supersymmetric algebra closes on the Hamiltonian alone. I will briefly review the N=1 (two real supercharges) construction, and then introduce an N=2 family of field theories with four real supercharges and a holomorphic structure. I will show how this relatively simple construction exhibits some surprising properties: Mainly, the marginal subcases realize lines of quantum exact, interacting Lifshitz fixed points with vanishing beta functions in various space dimensions. Additionally, these theories enjoy a rich moduli space of vacua with spontaneously broken translation symmetry.
10:45
Coffee
Coffee
10:45 - 11:15
11:15
Non-relativistic gravity and strings
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Niels Obers
Non-relativistic gravity and strings
Niels Obers
11:15 - 12:00
I will start by motivating the recent interest in non-relativistic gravity and strings, and introduce the basics of Newton-Cartan geometry. Newton-Cartan (NC) geometry was introduced more than 90 years ago in order to find a geometric formulation of Newtonian gravity. This geometry (including recent novel generalisation and extensions) has gained renewed interest as it appears in a variety of settings in modern theory involving gravity, string theory and holography. I will then talk about recent work on an action principle for non-relativistic gravity, including its Newtonian limit. This requires a new notion of NC geometry, which naturally arises in a covariant 1/c expansion of general relativity, with c being the speed of light. The corresponding truncation of general relativity yields a non-relativistic gravity theory that goes beyond Newtonian gravity and is able to correctly describe gravitational time dilation. Finally, I will discuss the relevance and appearance of non-relativistic geometry in connection with non-relativistric string theory and holography.
12:10
Non-relativistic Strings from Quantum Mechanics
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Troels Harmark
Non-relativistic Strings from Quantum Mechanics
Troels Harmark
12:10 - 12:55
This talk is about a new type of string theory with a non-relativistic conformal field theory on the world-sheet, as well as a non-relativistic target space geometry. Starting with the relativistic Polyakov action with a fixed momentum along a non-compact null-isometry, we can take a scaling limit that gives the non-relativistic string, including an interesting intermediate step. This can in particular be applied to a string on AdS5 x S5. In this case the scaling limit realizes a limit of AdS/CFT that on the field theory side gives a quantum mechanical theory known as Spin Matrix theory. We review that Spin Matrix theory is a finite-N version of nearest neighbor spin chains, from which one can find a long-wavelength semi-classical description using sigma-model such as the Landau-Lifshitz sigma-model. Hence, we can show that both sides of the AdS/CFT gives, in this limit, equivalent non-relativistic sigma-models that we are able to write down in a fully covariant manner, and show that it has a non-relativistic local symmetry that realizes the Galilean Conformal Algebra (GCA). This suggests that one has a holographic duality between the quantum mechanical theory of Spin Matrix theory, and the non-relativistic string. This could provide a more tractable holographic duality in which one can study the emergence of non-relativistic strings, geometry and gravity.
13:00
Lunch
Lunch
13:00 - 14:30
14:30
Entanglement measures in generalised quantum Lifshitz models
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Valentina Giangreco Puletti
Entanglement measures in generalised quantum Lifshitz models
Valentina Giangreco Puletti
14:30 - 15:15
The talk focusses on the computation and analysis of entanglement measures in generalised quantum Lifshitz models. These are free field theories with Lifshitz scaling symmetry which extend the (2+1)-dimensional quantum Lifshitz model to higher dimension, and provide us with simple models for non-relativistic critical theories. I will introduce various entanglement measures, such as entanglement entropy and logarithmic negativity (suitable to characterising quantum entanglement for pure and mixed states respectively), outline their computation in generalised quantum Lifshitz theories, and discuss the results.
15:15
Tea
Tea
15:15 - 15:45
15:45
Non-relativistic supersymmetry on curved backgrounds
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Jan Rosseel
Non-relativistic supersymmetry on curved backgrounds
Jan Rosseel
15:45 - 16:30
In this talk, I will briefly review how curved Riemannian manifolds, on which relativistic supersymmetric field theories can be defined, are found by studying a suitable set of differential Killing spinor equations. These Killing spinor equations are determined by the supersymmetry transformation rules of the fermionic fields of off-shell relativistic supergravity. I will then argue that one can obtain curved Newton-Cartan backgrounds, on which non-relativistic supersymmetric field theories can be put, by studying a set of non-relativistic Killing spinor equations, that include both algebraic and differential equations. Finally, some examples and properties of these curved backgrounds will be discussed.