Geometric Foundations of Gravity in Tartu

Schedule

08:00
09:00
10:00
11:00
12:00
13:00
14:00
15:00
16:00
17:00
18:00
19:00
20:00
21:00
Cárdenas Muñoz
Time:Sunday, 00:00-00:00
Room:
Speaker:Iván Antonio Cárdenas Muñoz
Affiliation:Universidad de Sonora (Hermosillo, Mexico)
Title:Variation of the fine structure constant
Opening
Time:Monday, 09:00-09:15
Room:B103
Speaker:Official Opening
Title:Opening words by selected representatives
Odintsov
Time:Monday, 09:15-10:15
Room:B103
Speaker:Sergei D. Odintsov
Affiliation:Institut de Ciencies de lEspai (Barcelona, Spain)
Title:Unified inflation with late-time acceleration in higher-derivative gravity
Capozziello
Time:Monday, 10:45-11:45
Room:B103
Speaker:Salvatore Capozziello
Affiliation:University of Napoli "Federico II" (Naples, Italy)
Title:Addressing the missing matter problem in galaxies through a new fundamental gravitational radius
Cisterna
Time:Monday, 13:15-13:40
Room:A101
Speaker:Adolfo Cisterna
Affiliation:Universidad Central de Chile (Santiago de Chile, Chile)
Title:Neutron stars in Galileon models
Capoferri
Time:Monday, 13:15-13:40
Room:A102
Speaker:Matteo Capoferri
Affiliation:University College London (London, Great Britain)
Title:Hyperbolic propagator in curved space: an explicit global formula
Maki
Time:Monday, 13:40-14:05
Room:A101
Speaker:Takuya Maki
Affiliation:Nikaido-gakuen (Tokyo, Japan)
Title:Gravitational waves in GR-GSG hybrid theory of gravity
Fröb
Time:Monday, 13:40-14:05
Room:A102
Speaker:Markus Fröb
Affiliation:University of York (York, Great Britain)
Title:Gauge-invariant observables in perturbative quantum gravity
Morita
Time:Monday, 14:05-14:30
Room:A101
Speaker:Masaaki Morita
Affiliation:Okinawa National College of Technology (Okinawa, Japan)
Title:Post-Newtonian parameter in $f(R)$ gravity for late-time cosmology
Culetu
Time:Monday, 14:05-14:30
Room:A102
Speaker:Hristu Culetu
Affiliation:Ovidius University (Constanta, Romania)
Title:Semiclassical corrections to a regularized Schwarzschild metric
Vernov
Time:Monday, 14:55-15:20
Room:A101
Speaker:Sergey Vernov
Affiliation:Lomonosov Moscow State University (Moscow, Russia)
Title:Non-monotonic behaviour of the Hubble parameter in bouncing models with scalar fields
Golovnev
Time:Monday, 14:55-15:20
Room:A102
Speaker:Alexey Golovnev
Affiliation:Saint Petersburg State University (Saint Petersburg, Russia)
Title:Square roots of matrices in massive gravity
Vilson
Time:Monday, 15:20-15:45
Room:A101
Speaker:Ott Vilson
Affiliation:University of Tartu (Tartu, Estonia)
Title:The approximated scalar field equation and its transformation in scalar-tensor gravity
Blixt
Time:Monday, 15:20-15:45
Room:A102
Speaker:Daniel Blixt
Affiliation:Stockholm University (Stockholm, Sweden)
Title:Hamiltonian analysis of spin-2 fields with derivative interaction
Rünkla
Time:Monday, 15:45-16:10
Room:A101
Speaker:Mihkel Rünkla
Affiliation:University of Tartu (Tartu, Estonia)
Title:A frame independent classification of single field inflationary models
Kocic
Time:Monday, 15:45-16:10
Room:A102
Speaker:Mikica Kocic
Affiliation:Stockholm University (Stockholm, Sweden)
Title:Geometry of the interaction term in ghost-free bimetric theory
Malek
Time:Monday, 16:35-17:00
Room:A101
Speaker:Tomas Malek
Affiliation:Czech Academy of Sciences (Prague, Czech Republic)
Title:Universal metrics
Raidal
Time:Monday, 16:35-17:00
Room:A102
Speaker:Martti Raidal
Affiliation:National Institute of Chemical Physics and Biophysics (Tallinn, Estonia)
Title:Phenomenology of Dark Matter in Bigravity
Ortaggio
Time:Monday, 17:00-17:25
Room:A101
Speaker:Marcello Ortaggio
Affiliation:Czech Academy of Sciences (Prague, Czech Republic)
Title:Universal electromagnetic fields
Hohmann
Time:Monday, 17:00-17:25
Room:A102
Speaker:Manuel Hohmann
Affiliation:University of Tartu (Tartu, Estonia)
Title:Post-Newtonian limit of massive bimetric and scalar-tensor gravity
Obukhov
Time:Tuesday, 09:15-10:15
Room:B103
Speaker:Yuri Obukhov
Affiliation:Russian Academy of Sciences (Moscow, Russia)
Title:Poincare gauge gravity: An overview
Hehl
Time:Tuesday, 10:45-11:45
Room:B103
Speaker:Friedrich W. Hehl
Affiliation:University of Cologne (Cologne, Germany)
Title:Nonlocal gravity simulates dark matter
Giulini
Time:Tuesday, 13:15-13:40
Room:B103
Speaker:Domenico Giulini
Affiliation:Leibniz University of Hannover (Hannover, Germany)
Title:Space-Time Symmetries and Energy-Momentum Tensors
Tucker
Time:Tuesday, 13:40-14:05
Room:B103
Speaker:Robin Tucker
Affiliation:Lancaster University (Lancaster, Great Britain)
Title:On Gravitational Chirality as the Genesis of Astrophysical Jets
Favaro
Time:Tuesday, 14:05-14:30
Room:B103
Speaker:Alberto Favaro
Affiliation:Imperial College London (London, Great Britain)
Title:The singular geometry of electromagnetic wave propagation
Siemssen
Time:Tuesday, 14:55-15:20
Room:B103
Speaker:Daniel Siemssen
Affiliation:University of Warsaw (Warsaw, Poland)
Title:Quantization of Pre-Metric Electrodynamics and Quantum Inequalities
Itin
Time:Tuesday, 15:20-15:45
Room:B103
Speaker:Yakov Itin
Affiliation:Hebrew University (Jerusalem, Israel)
Title:Premetric gravity with a local and linear constitutive law
Ni
Time:Tuesday, 15:45-16:10
Room:B103
Speaker:Wei-Tou Ni
Affiliation:National Tsing Hua University (Hsinchu, Taiwan)
Title:Equivalence principles and Pre-Metric Formalisms
Vassiliev
Time:Tuesday, 16:35-17:00
Room:B103
Speaker:Dmitri Vassiliev
Affiliation:University College London (London, Great Britain)
Title:Gauge theory from an analyst's perspective
Boos
Time:Tuesday, 17:00-17:25
Room:B103
Speaker:Jens Boos
Affiliation:University of Alberta (Alberta, Canada)
Title:Curvature tensors in 4D Riemann-Cartan space
Schuller
Time:Wednesday, 09:15-10:15
Room:B103
Speaker:Frederic Schuller
Affiliation:University of Erlangen-Nuremberg (Erlangen, Germany)
Title:Gravitational Closure
Lämmerzahl
Time:Wednesday, 10:45-11:45
Room:B103
Speaker:Claus Lämmerzahl
Affiliation:University of Bremen (Bremen, Germany)
Title:An operational approach to General Relativity and issues beyond
Koivisto
Time:Thursday, 09:15-10:15
Room:B103
Speaker:Tomi S. Koivisto
Affiliation:Nordita (Stockholm, Sweden)
Title:Palatini theories of gravity
Pereira
Time:Thursday, 10:45-11:45
Room:B103
Speaker:Jose G. Pereira
Affiliation:São Paulo State University (São Paulo, Brazil)
Title:Selected Topics of Teleparallel Gravity
Ong
Time:Thursday, 13:15-13:40
Room:A101
Speaker:Yen Chin Ong
Affiliation:Shanghai Jiao Tong University (Shanghai, China)
Title:Degrees of Freedom in $f(T)$ Gravity
Negreanu
Time:Thursday, 13:15-13:40
Room:A102
Speaker:Carina Negreanu
Affiliation:University of Cambridge (Cambridge, Great Britain)
Title:A new route to Conformal Gravity and beyond
Dialektopoulos
Time:Thursday, 13:40-14:05
Room:A101
Speaker:Kostas Dialektopoulos
Affiliation:University of Napoli "Federico II" (Naples, Italy)
Title:Noether Symmetries in Generalized Nonlocal Teleparallel Theories of Gravity
Hölscher
Time:Thursday, 13:40-14:05
Room:A102
Speaker:Patric Hölscher
Affiliation:Bielefeld University (Bielefeld, Germany)
Title:Astrophysical Gravitational Waves in Conformal Gravity
Bahamonde
Time:Thursday, 14:05-14:30
Room:A101
Speaker:Sebastian Bahamonde
Affiliation:University College London (London, Great Britain)
Title:New classes of modified teleparallel gravity models
Veermäe
Time:Thursday, 14:05-14:30
Room:A102
Speaker:Hardi Veermäe
Affiliation:National Institute of Chemical Physics and Biophysics (Tallinn, Estonia)
Title:Wormhole solutions in conformal gravity
Krššák
Time:Thursday, 14:55-15:20
Room:A101
Speaker:Martin Krššák
Affiliation:University of Tartu (Tartu, Estonia)
Title:Bigravity aspect of modified teleparallel theories
Gürlebeck
Time:Thursday, 14:55-15:20
Room:A102
Speaker:Norman Gürlebeck
Affiliation:University of Bremen (Bremen, Germany)
Title:BOOST: A Satellite Mission to Test Lorentz Invariance
Järv
Time:Thursday, 15:20-15:45
Room:A101
Speaker:Laur Järv
Affiliation:University of Tartu (Tartu, Estonia)
Title:Flat spin connection for rotating spacetimes in teleparallel $f(T)$ gravity
Perlick
Time:Thursday, 15:20-15:45
Room:A102
Speaker:Volker Perlick
Affiliation:University of Bremen (Bremen, Germany)
Title:A general redshift formula in Finsler spacetimes
Said
Time:Thursday, 15:45-16:10
Room:A101
Speaker:Jackson Said
Affiliation:University of Malta (Msida, Malta)
Title:Stability of the flat FLRW metric in $f(T)$ gravity
Pfeifer
Time:Thursday, 15:45-16:10
Room:A102
Speaker:Christian Pfeifer
Affiliation:University of Tartu (Tartu, Estonia)
Title:The radar experiment in the standard model extension electrodynamics
Ualikhanova
Time:Thursday, 16:35-17:00
Room:A101
Speaker:Ulbossyn Ualikhanova
Affiliation:University of Tartu (Tartu, Estonia)
Title:Dynamical systems approach and generic properties of $f(T)$ cosmology
An
Time:Thursday, 16:35-17:00
Room:A102
Speaker:Rui An
Affiliation:Shanghai Jiao Tong University (Shanghai, China)
Title:Constraints on the dark matter and dark energy interactions from weak lensing bispectrum tomography
Toporensky
Time:Thursday, 17:00-17:25
Room:A101
Speaker:Alexey Toporensky
Affiliation:Sternberg Astronomical Institute (Moscow, Russia)
Title:Asymptotic cosmological regimes in scalar-torsion gravity with a perfect fluid
Pozdeeva
Time:Thursday, 17:00-17:25
Room:A102
Speaker:Ekaterina Pozdeeva
Affiliation:Lomonosov Moscow State University (Moscow, Russia)
Title:The inflationary scenarios in GUT and MSSM
Kijowski
Time:Friday, 09:15-09:45
Room:B103
Speaker:Jerzy Kijowski
Affiliation:Polish Academy of Sciences (Warsaw, Poland)
Title:Universality of the Einstein's theory of gravitation
Shima
Time:Friday, 09:45-10:15
Room:B103
Speaker:Kazanuri Shima
Affiliation:Saitama Institute of Technology (Fukaya, Japan)
Title:Nonlinear-supersymmetric general relativity and unity of nature
Panel Discussion
Time:Friday, 10:45-11:45
Room:B103
Speaker:General Panel Discussion
Title:What are the most important questions to be pursued?
Registration
Time:Monday, 08:20-09:00
Name:Registration
Information:The registration desk is located in the entrance hall of the Physicum.
Coffee
Time:Monday, 10:15-10:45
Name:Coffee
Information:Coffee / tea is served in the entrance hall of the Physicum.
Lunch
Time:Monday, 11:45-13:15
Name:Lunch
Information:Please check the map for lunch options.
Coffee
Time:Monday, 14:30-14:55
Name:Coffee
Information:Coffee / tea is served in the entrance hall of the Physicum.
Coffee
Time:Monday, 16:10-16:35
Name:Coffee
Information:Coffee / tea is served in the entrance hall of the Physicum.
Registration
Time:Tuesday, 08:45-09:15
Name:Registration
Information:The registration desk is located in the entrance hall of the Physicum.
Coffee
Time:Tuesday, 10:15-10:45
Name:Coffee
Information:Coffee / tea is served in the entrance hall of the Physicum.
Lunch
Time:Tuesday, 11:45-13:15
Name:Lunch
Information:Please check the map for lunch options.
Coffee
Time:Tuesday, 14:30-14:55
Name:Coffee
Information:Coffee / tea is served in the entrance hall of the Physicum.
Coffee
Time:Tuesday, 16:10-16:35
Name:Coffee
Information:Coffee / tea is served in the entrance hall of the Physicum.
Public Lecture
Time:Tuesday, 18:15-19:15
Name:Public Lecture
Information:The public lecture by Robin Tucker will take place in the Old Observatory.
Coffee / Posters
Time:Wednesday, 10:15-10:45
Name:Coffee / Posters
Information:Coffee / tea is served in the entrance hall of the Physicum. If you present a poster, please be at your poster during this coffee break, so that people can ask questions.
Lunch
Time:Wednesday, 11:45-13:15
Name:Lunch
Information:Please check the map for lunch options.
Coffee / Posters
Time:Thursday, 10:15-10:45
Name:Coffee / Posters
Information:Coffee / tea is served in the entrance hall of the Physicum. If you present a poster, please be at your poster during this coffee break, so that people can ask questions.
Lunch
Time:Thursday, 11:45-13:15
Name:Lunch
Information:Please check the map for lunch options.
Coffee
Time:Thursday, 14:30-14:55
Name:Coffee
Information:Coffee / tea is served in the entrance hall of the Physicum.
Coffee
Time:Thursday, 16:10-16:35
Name:Coffee
Information:Coffee / tea is served in the entrance hall of the Physicum.
Coffee
Time:Friday, 10:15-10:45
Name:Coffee
Information:Coffee / tea is served in the entrance hall of the Physicum.
Lunch
Time:Friday, 11:45-13:15
Name:Lunch
Information:Please check the map for lunch options.
invited talk
scalar-tensor gravity
massive and bimetric gravity
conformal gravity
gauge theory
Lorentz violation and Finsler geometry
mathematical and quantum gravity
foundations of teleparallel gravity
teleparallel cosmology
other topics

Iván Antonio Cárdenas Muñoz (Universidad de Sonora, Hermosillo, Mexico):

Variation of the fine structure constant

We evaluate the fine structure constant variation which should take place as the Universe expands and its curvature is changed adiabatically. This variation of the fine structure constant is attributed to an energy losses by the physical system (consist of baryonic component and electromagnetic field) due to expansion of our Universe. Obtained ratio which is only five times smaller than actually reported experimental limit on this value. For this reason this variation can probably be measured within a couple of years. To argue the correctness of our approach we calculate the Planck constant as adiabatic invariant of electromagnetic field in the framework of the pseudo- Riemannian geometry.

Monday
08:20-09:00

Registration

The registration desk is located in the entrance hall of the Physicum.

B103
09:00-09:15

Official Opening:

Opening words by selected representatives

09:15-10:15

Sergei D. Odintsov (Institut de Ciencies de lEspai, Barcelona, Spain):

Unified inflation with late-time acceleration in higher-derivative gravity

We review the consistent universe evolution unifying inflation with late-time acceleration in modified gravity. As first example the modified $F(R)$ gravity is considered. The account of quantum effects to this scenario is done via inclusion of the conformal anomaly. Finally, the early-time accelerating universe is presented in frames of higher-derivative quantum gravity. Several possibilities for realistic inflation are considered. The consistent and realistic unification of inflation with dark energy with account of quantum gravity corrections in modified gravity is given. Unlike to usual $F(R)$ gravity, the problem of past oscillations does not occur there.
These results are based mainly on the following works:

1. Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
S. Nojiri, S.D. Odintsov, V.K. Oikonomou. Phys.Repts., to appear. 119 pp.
e-Print: arXiv:1705.11098

2. Beyond-one-loop quantum gravity action yielding both inflation and late-time acceleration
E. Elizalde, S.D. Odintsov, L. Sebastiani, R. Myrzakulov.NPB, to appear,
e-Print: arXiv:1706.01879

10:15-10:45

Coffee

Coffee / tea is served in the entrance hall of the Physicum.

10:45-11:45

Salvatore Capozziello (University of Napoli "Federico II", Naples, Italy):

Addressing the missing matter problem in galaxies through a new fundamental gravitational radius

We demonstrate that the existence of a Noether symmetry in $f(R)$ theories of gravity gives rise to a further gravitational radius, besides the standard Schwarzschild one, determining the dynamics at galactic scales. By this feature, it is possible to explain the baryonic Tully–Fisher relation and the rotation curve of gas-rich galaxies without the dark matter hypothesis.

11:45-13:15

Lunch

Please check the map for lunch options.

A101
A102
13:15-13:40

Adolfo Cisterna (Universidad Central de Chile, Santiago de Chile, Chile):

Neutron stars in Galileon models

During this talk we will present some results related to the construction of static and slowly rotating neutron stars in the context of galileon scalar-tensor theories.

Matteo Capoferri (University College London, London, Great Britain):

Hyperbolic propagator in curved space: an explicit global formula

In my talk I will discuss how it is possible to approximate the propagator for the wave operator on an arbitrary Riemannian manifold by means of a single oscillatory integral, global both in space and in time. The method is fully explicit and it allows, thanks to the adoption of a complex-valued phase function, to circumvent the topological obstruction of the underlying manifold known to prevent a construction global in time. The result naturally extends to globally hyperbolic space-times and it can be applied to Maxwell systems and the Dirac operator to describe the propagation of elementary particles, such as neutrinos and electrons, in relativistic settings. Joint work with Dmitri Vassiliev.

13:40-14:05

Takuya Maki (Nikaido-gakuen, Tokyo, Japan):

Gravitational waves in GR-GSG hybrid theory of gravity

In the last year, GR-GSG hybrid theory of gravity was proposed by Kan, Maki and Shiraishi. We study the perturbations in the theory and discuss the gravitational waves.

Markus Fröb (University of York, York, Great Britain):

Gauge-invariant observables in perturbative quantum gravity

It is well known that the diffeomorphism invariance of gravitational theories makes it impossible to define local and gauge-invariant observables in perturbative (quantum) gravity, except at linear order. While in flat space on can study the S-Matrix, which is a gauge-invariant global observable, no analogue exists in a general curved space. Relational observables (i.e., the value of one field at the point where a second field has a prescribed value) are natural candidates for observables in (quantum) gravity, but they are not local when constructed around flat space or around a cosmological (FLRW) background spacetime due to the high symmetry of the latter. We present two different approaches to this problem: a) correlation functions at fixed geodesic distance, and b) a construction of invariant coordinates, for which explicit and fully renormalized results for one-graviton-loop corrections to two-point functions and coupling constants have been obtained.

14:05-14:30

Masaaki Morita (Okinawa National College of Technology, Okinawa, Japan):

Post-Newtonian parameter in $f(R)$ gravity for late-time cosmology

We derive a formula for the post-Newtonian parameter $\gamma$ in $f(R)$ gravity in a straightforward manner without using a scalar-tensor representation or the transformation to the Einstein frame. We employ a cosmological post-Newtonian approximation, in which two small parameters, $\epsilon := v/c$ (peculiar velocity devided by the speed of light) and $\kappa := \ell / \ell_{H}$ (scale of cosmic inhomogeneities devided by the Hubble horizon scale) are introduced. A careful order-of-magnitude estimate of each term in the field equations is made with $\epsilon$ and $\kappa$ for the derivation. This approximation enables us to treat local-scale high-density regions, in which the chameleon mechanism would take place. Our results update the previously known ones and provide more stringent constraints from local gravity tests than before.

Hristu Culetu (Ovidius University, Constanta, Romania):

Semiclassical corrections to a regularized Schwarzschild metric

A version of the Schwarzschild metric to be valid in microphysics is proposed. The source fluid is anisotropic with $p_{r} = −\rho$ and fluctuating tangential pressures. At large distances with respect to the Compton wavelength associated to the source particle, they do not depend on the mass m of the source and everywhere depend on $\hbar$ and the velocity of light $c$ but not on the Newton constant $G$. The particle may be a black hole for $m > m_{P}$ only and when $m = m_{P}$ becomes an extremal black hole. The Komar energy $W$ of the gravitational fluid is $mc^{2}$ for $\hbar = 0$ and at large distances and vanishes at $r_{0} = 2\hbar/emc$. The WEC is violated when $r < r_{0}/2$ due to the negative tangential pressures.

14:30-14:55

Coffee

Coffee / tea is served in the entrance hall of the Physicum.

14:55-15:20

Sergey Vernov (Lomonosov Moscow State University, Moscow, Russia):

Non-monotonic behaviour of the Hubble parameter in bouncing models with scalar fields

We explore dynamics of cosmological models with bounce solutions evolving on a spatially flat FLRW background. We consider cosmological models with non-minimally coupled scalar fields and polynomial potentials. In particular, the model that contains the Hilbert-Einstein curvature term, the conformal coupling term and the Higgs-like potential with an opposite sign is studied in detail. Bounce solutions with non-monotonic Hubble parameters have been found and analysed. In this model the evolution of the Hubble parameter of the bounce solution essentially depends on the sign of the cosmological constant.

My talk is particularly based on the paper by E.O. Pozdeeva, M.A. Skugoreva, A.V. Toporensky, S.Yu. Vernov, JCAP 1612 (2016) no.12, 006 [arXiv:1608.08214]

Alexey Golovnev (Saint Petersburg State University, Saint Petersburg, Russia):

Square roots of matrices in massive gravity

The modern theory of ghost-free massive gravity hinges upon the notion of a square root of a matrix. This is non-trivial and not unique. It makes the standard perturbation theory in terms of matrices problematic, and in some cases even impossible. We describe the mathematics behind these issues, and offer a new method of dealing with massive gravity: in terms of eigenvalues instead of matrices.

15:20-15:45

Ott Vilson (University of Tartu, Tartu, Estonia):

The approximated scalar field equation and its transformation in scalar-tensor gravity

In this talk, by considering the Friedmann cosmology we introduce the general relativity regime of a scalar-tensor theory as a critical point in the 2-dimensional phase space of the scalar field. After approximating the scalar field equation around that point, we determine the possible attractor behaviour by studying the solutions. In these theories one is used to consider a frame transformation and a reparametrization of the scalar field. The latter might be singular at the general relativity regime, because for example in the Jordan frame Brans-Dicke parametrization the regime is determined by a diverging function, while in the Einstein frame canonical parametrization such a possibility does not occur at all. As the key result of this talk, we show that the nature of the critical point is preserved even under a singular reparametrization of the scalar field.

Daniel Blixt (Stockholm University, Stockholm, Sweden):

Hamiltonian analysis of spin-2 fields with derivative interaction

In Hassan-Rosen bimetric gravity the kinetic terms are given by two Einstein-Hilbert terms (one for each metric), with a specific form of the interaction potential, making the theory consistent. One can consider bimetric theories with derivative interactions and investigate with the Hamiltonian analysis if these are consistent theories. To do this, it is helpful to work in the vielbein formalism. I will highlight the crucial steps made for a couple of examples.

15:45-16:10

Mihkel Rünkla (University of Tartu, Tartu, Estonia):

A frame independent classification of single field inflationary models

Some unrelated models of inflation that originate from different physical setups yield, in some cases, identical predictions for the currently constrained inflationary observables. In order to classify the available models, we propose to express the slow-roll parameters and the relevant observables in terms of frame and reparametrisation invariant quantities. The adopted invariant formalism makes manifest the redundancy that afflicts the current description of inflation dynamics and offers a straightforward way to identify classes of models which yield identical phenomenology. As a main part of the talk we introduce a step-to-step recipe to recast every single field inflationary model in the proposed formalism, detailing also the procedure to compute inflationary observables in terms of invariant quantities.

Mikica Kocic (Stockholm University, Stockholm, Sweden):

Geometry of the interaction term in ghost-free bimetric theory

The absence of ghosts in bimetric theory is ensured by the special form of the interaction term that is based on the matrix square root function of the two metric fields combined. We present the theorem which connects this square root with the local causality in terms of the relation between the null-cones of the two metrics.

16:10-16:35

Coffee

Coffee / tea is served in the entrance hall of the Physicum.

16:35-17:00

Tomas Malek (Czech Academy of Sciences, Prague, Czech Republic):

Universal metrics

Universal metrics solve, by definition, vacuum field equations of all theories with the Lagrangian described by any polynomial curvature invariant constructed from the metric, the Riemann tensor and its covariant derivatives of arbitrary order. These metrics are thus insensitive to quantum corrections to the Einstein gravity. We study universal Lorentzian metrics of any dimension belonging to the Kundt class of non-expanding, non-shearing and non-twisting spacetimes. We also discuss Walker metrics of neutral signature admitting a field of parallel null 2-planes and identify universal metrics within this class.

Martti Raidal (National Institute of Chemical Physics and Biophysics, Tallinn, Estonia):

Phenomenology of Dark Matter in Bigravity

I review the problems related to the experimental searches for the Dark Matter of the Universe in particle physics and argue that the theories of bimetric and multimetric gravity offer viable alternatives. I explicitly work out two mechanism for massive spin-2 Dark Matter creation in those theories that cover its mass ranges from $10^{-23}$ eV to few TeV. I comment on experimentally testable aspects of those theories such as Dark Matter indirect detection in cosmic rays and Dark Matter direct detection in laboratory experiments.

17:00-17:25

Marcello Ortaggio (Czech Academy of Sciences, Prague, Czech Republic):

Universal electromagnetic fields

Already in the 30s, Schroedinger observed that all null Maxwell fields solve the equations for the electromagnetic field in any non-linear electrodynamics. More generally, we study properties of “universal” p-forms, i.e., electromagnetic fields that solve simultaneously any generalized electrodynamics (for which the field equations contain arbitrary powers and derivatives of the field strenght). Some results including the coupling to Einstein's gravity are also discussed, and analogies with “universal spacetimes” (which solve simultaneously virtually any theory of gravity) mentioned.

Manuel Hohmann (University of Tartu, Tartu, Estonia):

Post-Newtonian limit of massive bimetric and scalar-tensor gravity

In my talk I discuss the parametrised post-Newtonian (PPN) limit for spherically symmetric spacetimes in theories with additional massive degrees of freedom compared to the single metric present in general relativity. For the scalar-tensor theory, I will consider a homogeneous spherical mass source and discuss the relevance of the gravitational self energy for the PPN parameters gamma and beta. In particular, I will show that the limit of a vanishing source radius, for which the self energy diverges, is valid only for the linearised theory and the PPN parameter gamma. In this limit I will compare the result to the corresponding result for massive bimetric gravity, which has a second tensor field instead of a scalar field.

19:00-21:30
Tuesday
08:45-09:15

Registration

The registration desk is located in the entrance hall of the Physicum.

B103
09:15-10:15

Yuri Obukhov (Russian Academy of Sciences, Moscow, Russia):

Poincare gauge gravity: An overview

The talk presents the basics and the current status of the Poincare gauge gravity theory. After recalling the main geometric structures in the theory of the gravitational field, and giving a brief account of the history of the subject, an introduction to the gauge approach in the classical field theory is made along the lines of Yang-Mills and Utiyama-Kibble. The general dynamical scheme of the Poincare gauge (PG) gravity is formulated, which is then specialized to the Einstein-Cartan model and to the class of quadratic PG models.

10:15-10:45

Coffee

Coffee / tea is served in the entrance hall of the Physicum.

10:45-11:45

Friedrich W. Hehl (University of Cologne, Cologne, Germany):

Nonlocal gravity simulates dark matter

The analogy between electrodynamics and the translational gauge theory of gravity is employed to develop an ansatz for a nonlocal generalization of Einstein’s theory of gravitation. Working in the linear approximation, we show that the resulting nonlocal theory is equivalent to general relativity with dark matter. The nature of the predicted dark matter, which is the manifestation of the nonlocal character of gravity in our model, is briefly discussed. It is demonstrated that this approach can provide a basis for the Tohline-Kuhn treatment of the astrophysical evidence for dark matter.

Literature: F.W. Hehl and B. Mashhoon, Phys. Rev. D 79, 064028 (2009), B. Mashhoon, Nonlocal Gravity, Oxford University Press (2017).

11:45-13:15

Lunch

Please check the map for lunch options.

13:15-13:40

Domenico Giulini (Leibniz University of Hannover, Hannover, Germany):

Space-Time Symmetries and Energy-Momentum Tensors

In my talk I show how proper geometric formulations of symmetries and energy-momentum tensors eliminate conceptual uncertainties regarding globally conserved quantities and other integral relations, which usually are given in coordinate-dependent language that not only hide their geometric meaning, but also the hypotheses on which they implicitly rest.

13:40-14:05

Robin Tucker (Lancaster University, Lancaster, Great Britain):

On Gravitational Chirality as the Genesis of Astrophysical Jets

It has been suggested that single and double jets observed emanating from certain astrophysical objects may have a purely gravitational origin. I will discuss new classes of plane-fronted and pulsed gravitational wave solutions to the equation for perturbations of Ricci-flat spacetimes around Minkowski metrics, as models for the genesis of such phenomena. These solutions are classified in terms of their chirality and generate a family of non-stationary spacetime metrics. Particular members of these families are used as backgrounds in analysing time-like solutions to the geodesic equation for test particles. They are found numerically to exhibit both single and double jet-like features with dimensionless aspect ratios suggesting that it may be profitable to include such backgrounds in simulations of astrophysical jet dynamics from rotating accretion discs involving electromagnetic fields.

14:05-14:30

Alberto Favaro (Imperial College London, London, Great Britain):

The singular geometry of electromagnetic wave propagation

Premetric electrodynamics has provided clarity to different aspects of Maxwell’s theory, e.g. the study of vacuum birefringence, and the controversy on the definition of the energy-momentum tensor (Abraham vs. Minkowski). I will explain how the premetric formulation also brings order to research on anisotropic materials.

14:30-14:55

Coffee

Coffee / tea is served in the entrance hall of the Physicum.

14:55-15:20

Daniel Siemssen (University of Warsaw, Warsaw, Poland):

Quantization of Pre-Metric Electrodynamics and Quantum Inequalities

This talk concerns the quantization of the vector potential in pre-metric electrodynamics with a linear and local constitutive law. If the Fresnel polynomial associated to a constitutive law is hyperbolic, it gives rise to a causality structure which generalizes that of Lorentzian geometry. After a gauge fixing it  is then in many cases possible to construct the retarded and advanced Green’s functions. Their existence forms the basis of the algebraic quantization of the vector potential, as they appear in the commutation relations. In some cases even a ‘vacuum’ state can be found, thus leading to a full quantization. It is known on general grounds that in quantum field theory the pointwise energy density is unbounded from below. Suitably averaged over a region of spacetime or along a ‘timelike’ curve, the energy density can often be shown to be bounded below. This is a so-called quantum energy inequality (QEI). Thanks to the richer causality structure in pre-metric electrodynamics, also more possibilities for different QEIs arise. I will explain general results on QEIs for the pre-metric vector potential, as well as concrete calculations for uniaxial crystals.

15:20-15:45

Yakov Itin (Hebrew University, Jerusalem, Israel):

Premetric gravity with a local and linear constitutive law

In the standard formulation of general relativity (GR), the metric tensor serves as a primary field variable. This construction is in contrast to gauge theory in which a separation between the premetric field equations and a metric dependent constitutive relation is possible. In this talk, we demonstrate that GR allows for a premetric formulation, too. For this purpose, we apply the teleparallel approach of gravity, which represents GR as a gauge theory based on the translation group. We formulate the metric-free topological field equation and a general linear constitutive law between the basic field variables. The requirement of local Lorentz invariance turns the model into a full equivalent of GR. Our approach opens a way for a natural extension of GR to diverse geometrical structures of spacetime.

15:45-16:10

Wei-Tou Ni (National Tsing Hua University, Hsinchu, Taiwan):

Equivalence principles and Pre-Metric Formalisms

Pre-metric formalisms are general frameworks to test Einstein Equivalence Principle which is the basis of Metric (Pseudo-Riemannian) Geometry in the physical world. Galileo weak equivalence principle is a cornerstone of fundamental physics. We formulate Weak Equivalence Principles WEP I and WEP II for photons in the spirit of Galileo to explore the early universe and quantum gravity. Employing a 4-dimensional pre-metric formulation of electrodynamics of continuous medium and the validity of WEP I for photons (nonbirefringence), the spacetime structure must consist of a core metric field together with an axion field and a dilaton field. Since WEP I for photons is verified empirically to ultrahigh precision, the existence of core metric has been verified to second order in the ratio of Higgs mass to Planck mass. The extension of pre-metric framework to include skewons is formulated by Hehl and Obukhov. The extension of pre-metric framework to gravity part will be reported by Itin, Hehl and Obukhov. I will mention an extension to hyperspace unified theory. I dedicate this talk to Fred Hehl on his 80th birthday.

16:10-16:35

Coffee

Coffee / tea is served in the entrance hall of the Physicum.

16:35-17:00

Dmitri Vassiliev (University College London, London, Great Britain):

Gauge theory from an analyst's perspective

We work with a pair of complex-valued scalar fields over a 4-manifold. Our object of study is a first order Hermitian sesquilinear form, i.e. an integral over the manifold whose integrand is a linear combination of terms "product of gradient of scalar field and scalar field" and "product of two scalar fields". We call two sesquilinear forms equivalent if one is obtained from the other by some $x$-dependent $\mathrm{GL}(2,\mathbb{C})$ transformation, i.e. by a change of basis in the infinite-dimensional vector space of pairs of complex-valued scalar fields. Our aim is to provide an explicit description of equivalence classes of sesquilinear forms. We achieve this aim, and in doing this we show that our sesquilinear forms implicitly contain geometric constructs such as Lorentzian metric, spin structure, connection coefficients and electromagnetic covector potential.

The talk is based on DOI:10.1088/1751-8113/48/16/165203 and arXiv:1611.08297.

17:00-17:25

Jens Boos (University of Alberta, Alberta, Canada):

Curvature tensors in 4D Riemann-Cartan space

We present the irreducible decomposition of the curvature tensor in a spacetime with curvature and torsion, and discuss the corresponding notions of superenergy in form of a generalized Bel-Robinson tensor.

18:15-19:15

Public Lecture

The public lecture by Robin Tucker will take place in the Old Observatory.

Wednesday
B103
09:15-10:15

Frederic Schuller (University of Erlangen-Nuremberg, Erlangen, Germany):

Gravitational Closure

10:15-10:45

Coffee / Posters

Coffee / tea is served in the entrance hall of the Physicum. If you present a poster, please be at your poster during this coffee break, so that people can ask questions.

10:45-11:45

Claus Lämmerzahl (University of Bremen, Bremen, Germany):

An operational approach to General Relativity and issues beyond

Using as guideline the well known axiomatic approach to the geometry of space and time by Ehlers, Pirani and Schild, we show which experiments are needed to establish General Relativity. After having introduced the formalism of General Relativity its experimental consequences together with the corresponding observations/experiments are summarized. The talk ends by describing open fundamental issues, mainly related to the question of quantum mechanics and gravitation.

11:45-13:15

Lunch

Please check the map for lunch options.

13:15-21:00
Thursday
B103
09:15-10:15

Tomi S. Koivisto (Nordita, Stockholm, Sweden):

Palatini theories of gravity

In the Palatini variation, the metric and the connection are considered as independent fields. The presence of two connections, the one generated by the metric and the independent one, in general leads to a "hybrid" geometry.

In this talk, the Palatini variation is restricted to a flat geometry. This sets the torsion to propagate, and the dynamics of general relativity can be reproduced by the quadratic action with an additional Lorentz symmetry. In a geometry with neither curvature nor torsion, the inertial connection is given by a vector field, and the equivalent quadratic theory is determined by the requirement of an extra symmetry that allows to "disconnect", i.e. eliminate the vector.

The new, simplifying formulation shall be applied to explore more generic, non-equivalent teleparallel and "disconnected" theories, and promising results will be reported concerning theoretical consistency (covariance, field content) and phenomenology (the PPN limit, cosmology).

10:15-10:45

Coffee / Posters

Coffee / tea is served in the entrance hall of the Physicum. If you present a poster, please be at your poster during this coffee break, so that people can ask questions.

10:45-11:45

Jose G. Pereira (São Paulo State University, São Paulo, Brazil):

Selected Topics of Teleparallel Gravity

Some key points of teleparallel gravity will be discussed and clarified. The focus will be on the spin connection, which in teleparallel gravity represents inertial effects of the frame used to describe the solution.

11:45-13:15

Lunch

Please check the map for lunch options.

A101
A102
13:15-13:40

Yen Chin Ong (Shanghai Jiao Tong University, Shanghai, China):

Degrees of Freedom in $f(T)$ Gravity

A generic $f(T)$ gravity in its original formulation has 5 degrees of freedom, not all of which are present on a given spacetime background even under perturbations. The extra degrees of freedom appear to lead to problems such as superluminal propagation and ill-posedness of the Cauchy problem. There has since been discussions about the "remnant symmetry" of $f(T)$ gravity, and other ways to formulate the theory, with the hope of evading these problems. We discuss here in particular, the Lagrange multiplier formulation of $f(T)$ gravity, and its counting of degrees of freedom.

Carina Negreanu (University of Cambridge, Cambridge, Great Britain):

A new route to Conformal Gravity and beyond

First proposed in the 1990s, Conformal Gravity seems to be a promising starting point in developing an alternative to Einstein's Theory as it has a full metric structure associated with General Relativity with the added bonus of a local conformal symmetry that is characteristic to particle theories. In this talk we will discuss how one can recover Conformal Gravity for a static, spherically symmetric system by working in the 'extended' Weyl Gauge Theory. Although this setup does not employ the new Gauge Theory at its full potential, it is a first application of the theory and (as we will show) a very promising start. We will begin by explaining the possible shortcomings of using a strongly constrained metric as the Mannheim-Kazanas metric. Using a more general metric, we will look at vacuum solutions and show how one can recover the standard vacuum equations for Conformal Gravity. By employing a Palatini-type approach we will present the first viable solution that incorporates matter sources. Finally using the new formalism we will focus on test particle motion and discuss the implications on Solar System scales.

13:40-14:05

Kostas Dialektopoulos (University of Napoli "Federico II", Naples, Italy):

Noether Symmetries in Generalized Nonlocal Teleparallel Theories of Gravity

Both (modified) teleparallel and nonlocal, theories of gravity gained a lot of attention the last few years, especially in the field of cosmology. Their ability to reproduce many results from general relativity and, in addition, to describe effects, for which, up to now, exotic forms of matter/energy were invoked, made them very popular in the community. In this talk, I will introduce a new class of theories, called Generalized Nonlocal Teleparallel Theories (GNTT), with the effective lagrangian $\mathcal{L}\sim f(\square ^{-1}T, \square ^{-1}B),$ where $T$ is the torsion scalar and $B$ is a boundary term. More specifically, I will focus on their cosmologies and I will use the Noether Symmetry Approach, in order to find for which forms of the Lagrangian, the equations of motion remain invariant under point transformations. Cosmological solutions will be discussed, too.

Patric Hölscher (Bielefeld University, Bielefeld, Germany):

Astrophysical Gravitational Waves in Conformal Gravity

We investigate the gravitational radiation from binary systems in Conformal Gravity (CG) and Massive Conformal Gravity (MCG). For MCG we distinguish between a small and a large graviton mass. We derive the inhomogeneous linearized field equations for the metric. These are given by a massive higher-derivative Klein-Gordon equation. As a sample, we calculate the orbital decay for the well-measured binary system PSRJ1012+5307. With the graviton mass derived from the analysis of galaxy rotation curves, we can show that the radiated energy for CG and MCG with a small graviton mass is much smaller than in General Relativity (GR). This means that gravitational radiation is not effective and there has to be another mechanism to explain the shrinkage of the orbital period of binary systems. For MCG with a large graviton mass, the decrease of the orbital period is in agreement with the current data if we use the strongest constraints on the graviton mass.

14:05-14:30

Sebastian Bahamonde (University College London, London, Great Britain):

New classes of modified teleparallel gravity models

In this talk, a new class of modified teleparallel theory is presented. The action of this theory is constructed by a function of the irreducible parts of torsion $f(T_{\text{ax}}, T_{\text{ten}}, T_{\text{vec}})$, where $T_{\text{ax}}$, $T_{\text{ten}}$ and $T_{\text{vec}}$ are the axial, tensor and vector components of torsion. This is the most general (well-motivated) second order teleparallel theory of gravity that can be constructed from the torsion tensor. Different particular second order theories can be recovered from this theory as new general relativity, conformal teleparallel gravity or $f(T)$ gravity. Additionally, the boundary term $B$ which connects the Ricci scalar with the torsion scalar via $R = −T + B$ is also incorporated in the action. By performing a conformal transformation, I will show that the unique theories which have an Einstein frame are either TEGR or $f(−T + B) = f(R)$ as expected. In this presentation, I will also discuss about the issue of the violation of the local Lorentz transformations within these theories.

Hardi Veermäe (National Institute of Chemical Physics and Biophysics, Tallinn, Estonia):

Wormhole solutions in conformal gravity

14:30-14:55

Coffee

Coffee / tea is served in the entrance hall of the Physicum.

14:55-15:20

Martin Krššák (University of Tartu, Tartu, Estonia):

Bigravity aspect of modified teleparallel theories

I will briefly review the variational problem in teleparallel gravity and show how it can lead to consistent formulation of modified theories. Particularly, I will focus on the case of $f(T)$ gravity, where this variation provides us with six additional field equations. Then I will argue that we can interpret modified teleparallel theories as effectively bigravity theories with two tetrads.

Norman Gürlebeck (University of Bremen, Bremen, Germany):

BOOST: A Satellite Mission to Test Lorentz Invariance

The proposed BOOst Symmetry Test (BOOST) mission will perform a test of the Lorentz Invariance by carrying out a Kennedy-Thorndike type experiment in space. It consists of two frequency references, where one is based on an optical resonator and the other frequency reference is based on a hyperfine transition in molecular iodine. They will reach instabilities below the $10^{-15}$ level at orbit averaging time. In the presentation, we summarize the mission and the suggested experimental setup briefly. The main focus of the presentation will be the science case formulated in different test theories: The Standard Model Extension, the Robertson-Mansouri-Sexl test theory, and for varying fundamental constants. We will show that an improvement of one to two orders of magnitude of the current-best constraints is feasible with the suggested setup.

15:20-15:45

Laur Järv (University of Tartu, Tartu, Estonia):

Flat spin connection for rotating spacetimes in teleparallel $f(T)$ gravity

In order to solve the field equations for a tetrad in covariant teleparallel $f(T)$ gravity, one needs to know the corresponding flat spin connection. The talk presents preliminary results on finding such spin connection for generic ansatz tetrad of axially symmetric rotating spacetime in Weyl canonical and Boyer-Lindquist coordinates. By a suitable local Lorentz transformation the spin connection can be made to vanish, while the respective tetrad becomes nondiagonal. From the procedure we may draw some conclusions on how to find a flat spin connection that satisfies the variational principle in $f(T)$ gravity in general.

Volker Perlick (University of Bremen, Bremen, Germany):

A general redshift formula in Finsler spacetimes

In this talk I'll present a general redshift formula in Finsler spacetimes. The formula is universal in the sense that it holds for any two observers (emitter and receiver) on a Finsler spacetime that is arbitrary except for the fact that is should satisfy some regularity conditions. As an illustration, the formula is then applied to observers (i) in certain spherically symmetric and static Finsler spacetimes, and (ii) in certain cosmological Finsler spacetime. -- This is joint work with Wolfgang Hasse (TU Berlin).

15:45-16:10

Jackson Said (University of Malta, Msida, Malta):

Stability of the flat FLRW metric in $f(T)$ gravity

$f(T)$ Gravity represents one of the leading alternatives to general relativity. It describes gravitation by means of torsion rather than curvature effects. Moreover, it has shown promise of explaining some of the outstanding problems in modern cosmology. In this talk, the stability of the theory is shown for two prominent torsional lagrangians. This is achieved by taking perturbations of the Hubble and energy density. A particular emphasis on the resulting state parameters for either case. Stability is important because it not only shows more about the behaviour of the underlying theory but can help constrain the particular models within the cosmological context.

Christian Pfeifer (University of Tartu, Tartu, Estonia):

The radar experiment in the standard model extension electrodynamics

The so called Standard Model Extension (SME) investigates the phenomenological influence of non-Lorentz invariant modifications of the Lagrangians of the standard model. We consider SME electrodynamics from a relativists point of view using the framework of pre-metric electrodynamics, the analysis of modified dispersion relations and Finsler Lagrangians.

We demonstrate that SME electrodynamics is a pre-metric theory of electrodynamics with bi-metric Fresnel polynomial. The latter defines the causal structure and dispersion relation of the theory from which we derive the corresponding point particle Finsler Lagrangian. As observable effect we calculate the radar experiment on SME electrodynamics Finsler spacetimes.

16:10-16:35

Coffee

Coffee / tea is served in the entrance hall of the Physicum.

16:35-17:00

Ulbossyn Ualikhanova (University of Tartu, Tartu, Estonia):

Dynamical systems approach and generic properties of $f(T)$ cosmology

We present a systematic analysis of the dynamics of flat Friedmann-Lema\^{i}tre-Robertson-Walker cosmological models with radiation and dust matter in generalized teleparallel $f(T)$ gravity. We show that the cosmological dynamics of this model is fully described by a function \(W(H)\) of the Hubble parameter, which is constructed from the function \(f(T)\). After reducing the phase space to two dimensions we derive the conditions on \(W(H)\) for the occurrence of de Sitter fixed points, accelerated expansion, crossing the phantom divide, and finite time singularities. Depending on the model parameters it is possible to have a bounce (from contraction to expansion) or a turnaround (from expansion to contraction), but cyclic or oscillating scenarios are prohibited. As an illustration of the formalism we consider power law $f(T) = T + \alpha(-T)^n$ models, and show that these allow only one period of acceleration and no phantom divide crossing.

This talk is based on the article Phys. Rev. D 96 (2017) 043508 [arXiv:1706:02376 [gr-qc]].

Rui An (Shanghai Jiao Tong University, Shanghai, China):

Constraints on the dark matter and dark energy interactions from weak lensing bispectrum tomography

We estimate uncertainties of cosmological parameters for phenomenological interacting dark energy models using weak lensing convergence power spectrum and bispectrum. We focus on the bispectrum tomography and examine how weak lensing bispectrum tomography can constrain the interaction between dark sectors, as well as other cosmological parameters. Employing the Fisher matrix analysis, we forecast uncertainties of the parameters in our models and find that the lensing bispectrum measurement can constrain the coupling parameters $\Delta\lambda_1\simeq 0.07$, $\Delta\lambda_2\simeq 0.02$ or even tighter if the equation of state of dark energy is set to be a constant. The cosmic shear will be measured from upcoming weak lensing surveys with high sensitivity, thus it enables us to use the higher order correlation functions of weak lensing to constrain the interaction between dark sectors and will potentially provide more stringent results with other observations combined.

17:00-17:25

Alexey Toporensky (Sternberg Astronomical Institute, Moscow, Russia):

Asymptotic cosmological regimes in scalar-torsion gravity with a perfect fluid

We consider cosmological dynamics of nonminimally coupled scalar field in the scalar-torsion gravity in the presence of a hydrodynamical matter. Potential of the scalar field have been chosen as power-law with negative index, this type of potentials is usually used in quintessence scenarios. We identify several asymptotic regimes, including de Sitter, kinetic dominance, kinetic tracker and tracker solution and study conditions for their existence and stability. We show that for each combination of coupling constant and potential power index one of regimes studied in the present paper is stable to the future.

Ekaterina Pozdeeva (Lomonosov Moscow State University, Moscow, Russia):

The inflationary scenarios in GUT and MSSM

The successful realization of the inflationary scenario for renormalization-group improved potentials corresponding to the Higgs sector of finite gauge models is possible with reasonable parameter values. It is shown that the model here constructed and Higgs-driven inflation belong to the same class of cosmological attractors. We analyze the inflationary scenarios which could be induced by the two-Higgs-doublet potential of the Minimal Supersymmetric Standard Model (MSSM) where five scalar fields have nonminimal couplings to gravity. Observables following from such MSSM-inspired multifield inflation are calculated and a number of consistent inflationary scenarios are constructed.

The report is based on Emilio Elizalde, Sergei D. Odintsov, Ekaterina O. Pozdeeva, Sergey Yu. Vernov JCAP 1602 (2016) 025 [arXiv:1509.08817], M. N. Dubinin, E. Yu. Petrova, E. O. Pozdeeva, M. V. Sumin, S. Yu. Vernov, MSSM-inspired multifield inflation, arXiv:1705.09624

19:00-21:30
Friday
B103
09:15-09:45

Jerzy Kijowski (Polish Academy of Sciences, Warsaw, Poland):

Universality of the Einstein's theory of gravitation

It is shown that generalizations of general relativity theory, which consist in replacing the (linear in scalar curvature) Hilbert Lagrangian by a generic scalar density depending upon the whole curvature tensor, are equivalent to the conventional Einstein theory for a (possibly) different metric tensor and (possibly) a different set of matter fields.

09:45-10:15

Kazanuri Shima (Saitama Institute of Technology, Fukaya, Japan):

Nonlinear-supersymmetric general relativity and unity of nature

Considering Riemann space-time inspired by nonlinear representation of SUSY(NLSUSY) whose tangent space possesses Grassmann $\mathrm{SL}(2,\mathbb{C})$ degrees of freedom besides the ordinary Minkowski ($\mathrm{SO}(1,3)$) ones and performing the ordinary geometric arguments of Einstein general relativity (GR) principle, we obtain NLSUSY invariant Einstein-Hilbert-type general relativity action (nonlinear supersymmetric general relativity (NLSUSYGR)) equipped with the cosmological term. NLSUSYGR would collapse spontaneously (Big Collapse) to ordinary Riemann space-time and Nambu-Goldstone fermion corresponding to $[\mathrm{superGL}(4,\mathbb{R})/\mathrm{GL}(4,\mathbb{R})]$ of Grassmann degrees of freedom. It gives a new paradigm for the SUSY unification of space-time and matter with the robust SUSY breaking encoded in space-time itself, where the standard model (SM) of the low energy particle physics can emerge in the true vacuum of NLSUSYGR as the effective theory composed of NG fermion. NLSUSYGR bridges between cosmology and particle physics.

10:15-10:45

Coffee

Coffee / tea is served in the entrance hall of the Physicum.

10:45-11:45

General Panel Discussion:

What are the most important questions to be pursued?

11:45-13:15

Lunch

Please check the map for lunch options.