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Understanding the small-scale structure of spacetime is one of the biggest challenges faced by modern theoretical physics. There are many different attempts to solve this problem and they reflect the diversity of approaches to quantum gravity. This workshop will bring together researchers from a wide range of quantum gravity approaches and give them an opportunity to exchange ideas and gain new insights.
Funding for this workshop has been provided by the Simons Foundation.
- Abhay Ashtekar, Pennsylvania State University
- Dorothea Bahns, University of Goettingen
- Beatrice Bonga, Perimeter Institute
- Steve Carlip, University of California, Davis
- Alejandra Castro, University of Amsterdam
- Lin-Qing Chen, Okinawa Institute of Science and Technology
- Cecilia Chirenti, Federal University of ABC
- Marina Cortes, University of Edinburgh
- Maïté Dupuis, Perimeter Institute
- Astrid Eichhorn, Heidelberg University & University of Southern Denmark
- Netta Engelhardt, Princeton University
- Valentina Forini, City Universtiy of London
- Flaminia Giacomini, Perimeter Institute
- Lisa Glaser, University of Vienna
- Ruth Gregory, Durham University
- Wei Li, Chinese Academy of Sciences
- Renate Loll, Radboud University of Nijmegen
- Catherine Meusburger, Friedrich-Alexander-Universität Erlangen-Nürnberg
- Sylvie Paycha, University of Postdam
- Nicola Pinamonti, University of Genova
- Mairi Sakellariadou, Kings College London
- Lee Smolin, Perimeter Institute
- Rafael Sorkin, Perimeter Institute
- Reiko Toriumi, Okinawa Institute of Science and Technology
- Yasaman Yazdi, Imperial College London
- Seth Asante, Perimeter Institute
- Sylvain Carrozza, Perimeter Institute
- Pierre Clavier, University of Potsdam
- Alfonso Garmendia, University of Potsdam
- Ian Jubb, Imperial College London
- Benjamin Knorr, Perimeter Institute
- Maria Julia Maristany, Perimeter Institute
- Melissa Rodriguez Zarate, Perimeter Institute
- Nitica Sakharwade, Perimeter Institute
- Krishan Saraswat, Perimeter Institute
- Barak Shoshany, Perimeter Institute
- Filip Simovic, Perimeter Institute & University of Waterloo
- Alexander Spies, Friedrich-Alexander-Universität Erlangen-Nürnberg
- Sebastian Steinhaus, Perimeter Institute
- Thomas Voss, Friedrich-Alexander-Universität Erlangen-Nürnberg
- Dianjun Zhao, Chinese Academy of Sciences
Monday, November 18, 2019
Time |
Event |
Location |
9:00 – 9:25am |
Registration |
Reception |
9:25 – 9:30am |
Bianca Dittrich, Perimeter Institute |
Bob Room |
9:30 – 10:20am |
Renate Loll, Radboud University of Nijmegen |
Bob Room |
10:20 – 11:10am |
Sylvie Paycha, University of Potsdam |
Bob Room |
11:10 – 11:40am |
Coffee Break |
Bistro – 1^{st} Floor |
11:40 – 12:30pm |
Reiko Toriumi, Okinawa Institute of Science and Technology |
Bob Room |
12:30 – 2:00pm |
Lunch |
Bistro – 2^{nd} Floor |
2:00 – 2:50pm |
Lee Smolin, Perimeter Institute |
Bob Room |
2:50 – 3:40pm |
Flaminia Giacomini, Perimeter Institute |
Bob Room |
3:40 – 4:10pm |
Coffee Break |
Bistro – 1^{st} Floor |
4:10 – 5:00pm |
Cecilia Chirenti, Federal University of ABC |
Bob Room |
5:00 - 5:50pm | Maïté Dupuis, Perimeter Institute | Bob Room |
Tuesday, November 19, 2019
Time |
Event |
Location |
9:30 – 10:20am |
Abhay Ashtekar, Pennsylvania State University |
Bob Room |
10:20 – 11:10am |
Astrid Eichhorn, |
Bob Room |
11:10 – 11:40am |
Coffee Break |
Bistro – 1^{st} Floor |
11:40 – 12:30pm |
Beatrice Bonga, Perimeter Institute |
Bob Room |
12:30 – 2:00pm |
Lunch |
Bistro – 2^{nd} Floor |
2:00 – 2:50pm |
Rafael Sorkin, Perimeter Institute |
Bob Room |
2:50 – 3:40pm |
Yasaman Yazdi, Imperial College London |
Bob Room |
3:40 – 4:10pm |
Coffee Break |
Bistro – 1^{st} Floor |
4:10 – 5:30pm |
Discussion on Quantum Gravity |
Bob Room |
Wednesday, November 20, 2019
Time |
Event |
Location |
9:30 – 10:20am |
Mairi Sakellariadou, Kings College London |
Bob Room |
10:20 – 11:10am |
Ruth Gregory, Durham University |
Bob Room |
11:10 – 11:40am |
Coffee Break |
Bistro – 1^{st} Floor |
11:40 – 12:30pm |
Alejandra Castro, University of Amsterdam |
Bob Room |
12:30 – 2:00pm |
Lunch |
Bistro – 2^{nd} Floor |
2:00 – 3:30pm |
Colloquium |
Theater |
3:30 – 4:00pm |
Coffee Break |
Bistro – 1^{st} Floor |
4:00 – 5:30pm |
Panel Discussion: Women in Science |
Sky Room |
6:00 – 9:00pm |
FemPhys Mentoring night |
Space Room |
Thursday, November 21, 2019
Time |
Event |
Location |
9:30 – 10:20am |
Dorothea Bahns, University of Goettingen |
Bob Room |
10:20 – 11:10am |
Nicola Pinamonti, University of Genova |
Bob Room |
11:10 – 11:40am |
Coffee Break |
Bistro – 1^{st} Floor |
11:40 – 12:30pm |
Valentina Forini, City University of London |
Bob Room |
12:30 – 2:00pm |
Lunch |
Bistro – 2^{nd} Floor |
2:00 – 2:50pm |
Steven Carlip, University of California, Davis |
Bob Room |
2:50 – 3:40pm |
Lisa Glaser, University of Vienna |
Bob Room |
3:40 – 4:10pm |
Coffee Break |
Bistro – 1^{st} Floor |
4:10 - 5:30pm | Gong Show | Bob Room |
6:00 – 9:00pm |
Banquet |
Bistro – 2^{nd} Floor |
Friday, November 22, 2019
Time |
Event |
Location |
9:30 – 10:20am |
Netta Engelhardt, Princeton University |
Bob Room |
10:20 – 11:10am |
Wei Li, Chinese Academy of Sciences |
Bob Room |
11:10 – 11:40am |
Coffee Break |
Bistro – 1^{st} Floor |
11:40 – 12:30pm |
Lin-Qing Chen, Okinawa Institute of Science and Technology |
Bob Room |
12:30 – 2:00pm |
Lunch |
Bistro – 2^{nd} Floor |
2:00 – 2:50pm |
Marina Cortes, University of Edinburgh |
Bob Room |
2:50 – 3:00pm |
Closing Remarks and Good-Bye |
Bob Room |
3:00 – 4:00pm |
Coffee Break |
Bistro – 1^{st} Floor |
Abhay Ashtekar, Pennsylvania State University
Implications of the Quantum Nature Space-time for the Big Bang and Black Holes
Dorothea Bahns, University of Goettingen
Quantum Sine-Gordon model in perturbative AQFT
We construct the Haag Kaster net of von Neumann algebras for the Sine-Gordon model. This is joint work with Klaus Fredenhagen and Kasia Rejzner.
Beatrice Bonga, Perimeter Institute
Angular momentum flux in Einstein-Maxwell theory
There are three natural currents for Maxwell theory on a non-dynamical background: the stress, Noether and canonical current. Their associated fluxes across null infinity differ by boundary terms for asymptotically flat spacetimes. These boundary terms do not only quantitatively change the behavior of the flux associated with an asymptotic Lorentz symmetry, but also qualitatively: the stress flux contains both radiative and Coulombic information, whereas Noether and canonical ones are purely radiative.
While all methods are equally valid and have their own range of usefulness, it is reasonable to ask if one definition is more natural than the other. In order to answer this question, we turn to general relativity. With Maxwell theory coupled to gravity, we use the Wald-Zoupas formalism to obtain an expression for the flux of angular momentum and find that it is purely radiative. When the gravitational field is ``frozen'', the Wald-Zoupas flux reduces to the Noether flux.
Steven Carlip, University of California, Davis
Spacetime Foam and the Cosmological Constant
I describe a radical proposal for the cosmological constant problem: perhaps Lambda really is very large, but is "hidden" in Planck-scale fluctuations of geometry and topology. I show that an enormous set of initial data describe a universe with such a hidden cosmological constant at an initial time. The question of whether this structure is preserved under time evolution is still open, but I provide some evidence that it may be. I close with a discussion of open questions that might lead to further insight (or perhaps kill the idea).
Alejandra Castro, University of Amsterdam
The Holographic Landscape of Symmetric Product Orbifolds
I will discuss the application of Siegel paramodular forms to constructing new examples of holography. These forms are relevant to investigate the growth of coefficients in the elliptic genus of symmetric product orbifolds at large central charge. The main finding is that the landscape of symmetric product theories decomposes into two regions. In one region, the growth of the low energy states is Hagedorn, which indicates a stringy dual. In the other, the growth is much slower, and compatible with the spectrum of a supergravity theory on AdS_3. I will provide a simple diagnostic which places any symmetric product orbifold in either region. The examples I will present open a path to novel realizations of AdS_3/CFT_2.
Lin-Qing Chen, Okinawa Institute of Science and Technology
Central extension and black hole entropy
Recent developments on asymptotic symmetries and soft modes have deepened our understanding of black hole entropy and the information paradox. The asymptotic symmetry charge algebra of certain classes of spacetimes could have a nontrivial central extension, which plays a crucial role in black hole physics. The Cardy formula of the asymptotic density of states of the dual CFT has been famously used to reproduce the Bekenstein-Hawking entropy formula. However, without assuming holography, it remains obscure from the point of view of gravity how such a constant on the gravitational phase space encodes the information about the density of black hole microstates, and what the gravitational degrees of freedom accounting for the black hole entropy truly are. I will discuss my ongoing efforts of understanding these questions in the covariant phase space formalism.
Cecilia Chirenti, Federal University of ABC
Probing fundamental physics with gravitational waves
According to general relativity, the coalescence of a compact binary system creates a gravitational wave signal generically described by an inspiral-merger-ringdown waveform. The recent observations of gravitational waves by LIGO allow us to test our theory of gravity in the strong field regime. In binary black hole detections, the ringdown portion of the wave can provide tests of the no-hair theorem, the most stringent proof of the existence of astrophysical black holes and even possible hints of quantum gravity. I will present the current status of these observations and discuss future prospects.
Marina Cortes, University of Edinburgh
Towards inclusion of biology in cosmology
Cosmologists wish to explain how our universe, in all its complexity, could ever have come about. For that, we assess the number degrees of freedom in our Universe now. This plays the role of entropy in thermodynamics of the Universe, and reveals the magnitude of the problem of initial conditions to be solved. In our budget, we account for gravity, thermal motions, and finally the vacuum energy whose entropy, given by the Bekenstein bound, dominates the entropy budget today.
There is however one number which we have not accounted for: the number of degrees of freedom in our complex biosphere. What is the entropy of life? Is it sizeable enough to need to be accounted for at the Big Bang, or negligible compared to vacuum entropy?
Astrid Eichhorn, Heidelberg University & University of Southern Denmark
The power of diversity - or why linking quantum gravity approaches could matter
Linking quantum gravity approaches could be important to make progress in quantum gravity. In my talk, I will try to make this case using asymptotically safe gravity as an example. I will briefly review the status of the approach and highlight the open questions, and discuss proposed ideas how the link to other approaches could be useful to tackle these. Finally, I will emphasize the need for universality in quantum gravity, and argue that there might be universal features from quantum gravity in black-hole shadows.
Netta Engelhardt, Princeton University
Evaporating Black Holes in AdS
Valentina Forini, City University of London
AdS/CFT and string sigma-model non-perturbatively
I will discuss progress on a non-perturbative approach to the study of string sigma-models relevant in AdS/CFT which exploits lattice field theory techniques.
Flaminia Giacomini, Perimeter Institute
Quantum reference frames for space and time
In physics, every observation is made with respect to a frame of reference. Although reference frames are usually not considered as degrees of freedom, in all practical situations it is a physical system which constitutes a reference frame. Can a quantum system be considered as a reference frame and, if so, which description would it give of the world? In the first part of my talk, I will introduce a general method to quantise reference frame transformations within a Galilean-relativistic setting, which generalises the usual reference frame transformation to a “superposition of coordinate transformations”. We describe states, measurement, and dynamical evolution in different quantum reference frames, without appealing to an external, absolute reference frame, and find that entanglement and superposition are frame-dependent features. The transformation also leads to a generalisation of the notion of covariance of dynamical physical laws. In the second part of my talk, I will show how these ideas can be used to operationally define the localization of events with respect to quantum clocks, each of which identifies a “time reference frame". In particular, I will consider clocks that i) are quantum mechanical, and ii) interact, gravitationally or otherwise, with other quantum systems. We find that, when gravitational effects are important, the time localisability of events becomes a relative concept, depending on the time reference frame. We discuss the physical significance of "jumping" onto a time reference frame with respect to which specific events are localised, in the context of indefinite causal structures arising from the interplay between quantum mechanics and gravity.
Lisa Glaser, University of Vienna
How much geometry is in a truncated spectral triple?
A spectral triple consists of an algebra, a Hilbert space and a Dirac operator, and if these three fulfill certain relations to each other they contain the entire information of a compact Riemannian manifold.
Using the language of spectral triples makes it possible to generalize the concept of a manifold to include non-commutativity.
While it is possible to write down finite spectral triples, often categorized as fuzzy spaces, that describe discretized geometries, classical geometries are encoded in infinite dimensional spectral triples. However working in numerical systems (and maybe ultimately in physical systems), only a finite part of this information can be encoded, which opens the question; If we know a part of the spectrum, how clearly can we characterise a geometry.
In this talk I will present first steps towards answering this question.
Ruth Gregory, Durham University
Tabletop Insights into Quantum Gravity?
I'll describe my recent work on black hole seeded vacuum decay, and proposals for testing seeded decay in cold atom experiments. I'll conclude with speculations on seeking insight into quantum black holes via experimentally constructing quantised analog black holes.
Wei Li, Chinese Academy of Sciences
Higher spin symmetry in gravity and string
Higher spin symmetries are gauge symmetries sourced by massless particles with spin greater than two. When coupled with diffeomorphism, they give rise to higher spin gravity. After a review on higher spin gravity, I will discuss its holography and its embedding in the string theory. Finally I will talk about some applications of higher spin symmetry, both in string theory and in QFT.
Renate Loll, Radboud University of Nijmegen
Quantum Spacetime from Lattice Gravity à la CDT
Causal Dynamical Triangulations (CDT) is a candidate theory for quantum gravity, formulated nonperturbatively as the scaling limit of a lattice theory in terms of triangulated spacetimes. An important feature of this approach is its elegant resolution of the problem of diffeomorphism symmetry in the full, background-free quantum theory. This has enabled the concrete computation of geometric observables in a highly nonperturbative, Planckian regime, an important step in putting quantum gravity on a quantitative footing, and understanding the structure of quantum spacetime. While the need to find quantum observables describing this regime is common to all approaches, CDT provides a concrete testing ground for implementation and measurements. In particular, a new notion of quantum Ricci curvature has opened a new window on the counterintuitive properties of quantum geometry.
Catherine Meusburger, Friedrich-Alexander-Universität Erlangen-Nürnberg
Ideal tetrahedra and their duals
This talk is based on joint work with Pierre Clavier, Li Guo and Bin Zhang
The dynamics of difference
A proposal is made for a fundamental theory, which is hypothesized to be a completion of both quantum mechanics and general relativity, in which the history of the universe is constituted of diverse views of itself. Views are attributes of events, and the theory’s only be-ables; they comprise information about energy and momentum transferred to an event from its causal past. A dynamics is proposed for a universe constituted of views of events, which combines the energetic causal set dynamics with a potential energy based on a measure of the distinctiveness of the views, called the variety. As in the real ensemble formulation of quantum mechanics, quantum pure states are associated to ensembles of similar events; the quantum potential of Bohm then arises from the variety.
This theory brings together results from two lines of development: energetic causal sets, developed with Marina Cortes, and the real ensemble formulation of quantum mechanics.
Closing Remarks and Good-Bye
Towards inclusion of biology in cosmology
Cosmologists wish to explain how our universe, in all its complexity, could ever have come about. For that, we assess the number degrees of freedom in our Universe now. This plays the role of entropy in thermodynamics of the Universe, and reveals the magnitude of the problem of initial conditions to be solved. In our budget, we account for gravity, thermal motions, and finally the vacuum energy whose entropy, given by the Bekenstein bound, dominates the entropy budget today.
Central extension and black hole entropy
Recent developments on asymptotic symmetries and soft modes have deepened our understanding of black hole entropy and the information paradox. The asymptotic symmetry charge algebra of certain classes of spacetimes could have a nontrivial central extension, which plays a crucial role in black hole physics. The Cardy formula of the asymptotic density of states of the dual CFT has been famously used to reproduce the Bekenstein-Hawking entropy formula.
Higher spin symmetry in gravity and string
Higher spin symmetries are gauge symmetries sourced by massless particles with spin greater than two. When coupled with diffeomorphism, they give rise to higher spin gravity. After a review on higher spin gravity, I will discuss its holography and its embedding in the string theory. Finally I will talk about some applications of higher spin symmetry, both in string theory and in QFT.
Evaporating Black Holes in AdS
How much geometry is in a truncated spectral triple?
A spectral triple consists of an algebra, a Hilbert space and a Dirac operator, and if these three fulfill certain relations to each other they contain the entire information of a compact Riemannian manifold.
Using the language of spectral triples makes it possible to generalize the concept of a manifold to include non-commutativity.
Spacetime Foam and the Cosmological Constant
I describe a radical proposal for the cosmological constant problem: perhaps Lambda really is very large, but is "hidden" in Planck-scale fluctuations of geometry and topology. I show that an enormous set of initial data describe a universe with such a hidden cosmological constant at an initial time. The question of whether this structure is preserved under time evolution is still open, but I provide some evidence that it may be. I close with a discussion of open questions that might lead to further insight (or perhaps kill the idea).
AdS/CFT and string sigma-model non-perturbatively
I will discuss progress on a non-perturbative approach to the study of string sigma-models relevant in AdS/CFT which exploits lattice field theory techniques.
Semiclassical Einstein equations in cosmological spacetimes
During this talk we shall discuss the backreaction of quantum matter fields on classical backgrounds by means of the semiclassical Einstein equation.
We shall see that self consistent solutions of this coupled system exist in the case of cosmological spacetimes.
Furthermore, Einstein equations governing the backreaction will transfer quantum matter fluctuations to the metric.
In particular, we will see how the singular structure of quantum matter will affect the spectrum of metric perturbations
Quantum Sine-Gordon model in perturbative AQFT
We construct the Haag Kaster net of von Neumann algebras for the Sine-Gordon model. This is joint work with Klaus Fredenhagen and Kasia Rejzner.
Pages
Scientific Organizers:
- Bianca Dittrich, Perimeter Institute
- Katarzyna Rejzner, University of York
- Sumati Surya, Raman Research Institute