Tunch available ()

Tunch available ()

Jenny Wagner (ITA, Heidelberg University)-

TBA

Tunch available ()

Alefe Almeida(ITP, Heidelberg University)

Group Discussion

Henrik Nersisyan

Quantum equivalence of f(R)-gravity and scalar-tensor-theories

Michael S. Ruf, Christian F. Steinwachs

e-Print: arXiv:1711.07486

Dario Bettoni

Vainshtein mechanism after GW170817

Marco Crisostomi, Kazuya Koyama

e-Print: arXiv:1711.06661

Adalto R. Gomes - UFMA (Brazil)- “Some results in kink-antikink scattering”

After introduced some motivations related to this topic (see for instance possible connections to bubble collisions [1]), I review some known results from kink-antikink scattering in nonintegrable models, focusing on the main aspects of the scalar field after the collision process: the formation of a bion state or inelastic scattering (1-bounce collision). The nonlinearity leads to the intriguing effect of 2-bounce collisions, observed for a range of initial velocities of the pair kink-antikink. This means that depending on the model, we can have the possibility of the formation of a structure of 2-bounce windows in velocity. Then I discuss a deformed $\phi^4$ model in (1,1) dimensions [2]. Stability analysis leads to a Schroedinger-like equation with a zero-mode and at least one vibrational (shape) mode. For small deformation and for one or two vibrational modes, the observed two-bounce windows in velocity are explained by the standard mechanism of a resonant effect between the first vibrational and the translational modes. With the increase of the deformation, the effect of the appearance of more than one vibrational mode is the gradual disappearance of the initial two-bounce windows. The total suppression of two-bounce windows even with the presence of a vibrational mode offers a counter-example of what expected from the standard mechanism [3]. I end presenting some recent results from kink-antikink scattering in a degenerate vacuum to vacuumless model [4].

[1] J. Braden, J. R. Bonda, L.Mersini-Houghtonc, “Cosmic bubble and domain wall instabilities I: parametric amplification of linear fluctuations”, JCAP03 (2015) 007.

[2] F. C. Simas, Adalto R. Gomes, K. Z. Nobrega, J.C.R.E. Oliveira, ”Suppression of two-bounce win- dows in kink-antikink collisions”, JHEP 1609 (2016) 104.

[3] D.K. Campbell, J.S. shonfeld, C.A. Wingate, “Resonance structure in kink-antikink interaction in $\phi^4$ theory”, Physica D 9 (1983) 1.

[4] F. C. Simas, Adalto R. Gomes, K. Z. Nobrega, “Degenerate vacua to vacuumless model and kink-antikink collisions”, Phys. Lett. B775 (2017) 290.

Cornelius Rampf

Solving the Vlasov equation in two spatial dimensions with the Schrödinger method

arXiv:1711.00140

Guillem Domenech

Stability of Geodesically Complete Cosmologies

arXiv:1610.04207

Lorenzo Pizzuti- “Modified gravity with galaxy cluster mass profiles: from data to simulations”

Abstract: I will provide a brief overview of my work concerning constraints on modified gravity models obtained using galaxy cluster mass profile determinations. In particular, I will present the results of a paper in which we combined the information given by the kinematics of galaxies in clusters with the information provided by lensing analyses for 2 galaxy clusters of the CLASH-CLASH\VLT collaboration to get constraints on f(R) models. In order to discuss the applicability of the proposed method in view of future imaging and spectroscopic surveys, I will further introduce my current study of cosmological simulations, aiming at estimating and calibrating the impact of systematics.

Adria Gomez-Valent

An alternative to the LCDM model: the case of scale invariance

arXiv arXiv:1701.03964

Special JC on Gravitational Waves detection

Caroline Heneka - Strong constraints on cosmological gravity from GW170817 and GRB 170817A - 1710.06394

Martin Pauly - GW170817 Falsifies Dark Matter Emulators - 1710.06168

Ana Marta Pinho - Welcome to the multi-messenger Era! Lessons from a neutron star and the landscape ahead - 1710.05931

Alessio Spurio Mancini - Dark Energy after GW170817 - 1710.05901

Martin Pauly (ITP, Heidelberg) - “Predictions of renormalized Higgs inflation”

Abstract: Higgs inflation is a model, that allows to explain inflation with the standard model degrees of freedom by introducing an additional coupling between the Higgs field and gravity. In this talk, I am going to explore the influence of the running of the standard model couplings on the observational predictions of Higgs inflation. In particular, the running of the Higgs-self-coupling and sudden changes in that coupling will be important. These sudden changes can be induced by the effective-field-theory nature of Higgs inflation. I will show that as long as the coupling stays sufficiently large in the inflationary region the predictions are insensitive to the running and become sensitive once the coupling approaches the critical point.

Caroline Heneka

Safely smoothing spacetime: backreaction in relativistic cosmological simulations

arXiv:1706.09309

Javier Rubio

Primordial Black Hole production in Critical Higgs Inflation

arXiv:1705.04861

Cornelius Rampf (ITP, Heidelberg University ) - “Shell-crossing in quasi one-dimensional flow ”

Abstract: So far exact analytic solutions to the cosmological fluid equations existed for initial data that only depend on one space variable. Exact solutions (until shell-crossing) play an important role in cosmology, not only because they are simple but because the breakdown of smooth 3D solution through the development of infinite density caustics begins generically as an almost 1D phenomenon with the formation of pancakes. I present recent work on quasi-one-dimensional (Q1D) flow that depends on all three coordinates but differs only slightly from a strictly 1D flow, thereby allowing a perturbative treatment of shell-crossing using the Euler-Poisson equations written in Lagrangian coordinates. The signature of shell-crossing is then just the vanishing of the Jacobian of the Lagrangian map, a regular perturbation problem. In essence, the problem of the first shell-crossing, which is highly singular in Eulerian coordinates, has been desingularized by switching to Lagrangian coordinates, and can then be handled by perturbation theory. All-order recursion relations are obtained for the time-Taylor coefficients of the displacement field, and it is shown that the Taylor series has an infinite radius of convergence. This allows the determination of the time and location of the first shell-crossing, which is generically shown to be taking place earlier than for the unperturbed 1D flow.

Caroline Heneka

Improving constraints on the growth rate of structure by modelling the density-velocity cross-correlation in the 6dF Galaxy Survey

arXiv:1706.05205

Santiago Casas (ITP, Heidelberg University) - “Non-linear structure formation”

Javier Rubio (ITP, Heidelberg University) - “Scale invariance: connecting inflation and dark energy”

Abstract: Inflation and dark energy share many essential properties. I will show that these two eras can be accommodated into a common framework based on scale invariance. I will discuss the phenomenological consequences of two scenarios based on i) exact scale symmetry and ii) broken scale invariance with symmetry resurgence at UV and IR fixed points.

Henrik Nersisyan

A Nonlocal Approach to the Cosmological Constant Problem

arXiv:1703.09715

Martin Pauly

Primordial black hole constraints for extended mass functions

arXiv:1705.05567

Alefe Almeida(ITP, Heidelberg University) - ” A method for evaluating models that use galaxy rotation curves to derive matter density profiles”

Abstract: There are some approaches, either based on GR or modified gravity that use galaxy rotation to derive the matter density of the corresponding galaxy. In this work, we proposed a test for evaluating them.

Kevin Wolz

Ana Marta Pinho

Stability of fundamental couplings: a global analysis

arXiv:1701.08724

Yves Dirian (Geneva University ) - “A numerical relativity scheme for cosmological simulations”

Abstract: I present a new 3+1 integration scheme which allows one to pass an adaptation of the robustness test to the cosmological context, at least in the case of General Relativity with a pressureless perfect fluid field. As an interesting by-product of this construction, a novel constraint-damping method is obtained.

Viviana Niro

Dario Bettoni

Gravitational Waves in Doubly Coupled Bigravity

arXiv:1703.08016