12:10 PM
|
Explaining the Hubble tension and dark energy from alpha-attractors
- Prof.
Konstantinos Dimopoulos
(Lancaster University)
|
12:30 PM
|
Cosmology under the fractional calculus approach: a possible $H_0$ tension resolution?
- Dr
Genly Leon
(Universidad Catolica del Norte)
|
12:50 PM
|
Solving tensions faster with velocities
- Prof.
Miguel Quartin
(Heidelberg U. + U. Federal do Rio de Janeiro)
|
1:10 PM
|
Tensions in Cosmological Probes and Quasar Cosmology
- Dr
Micol Benetti
(University of Naples)
|
1:30 PM
|
--- Lunch break ---
|
3:30 PM
|
Alleviation of H0 tension in f(Q) gravity
- Dr
Fotios Anagnostopoulos
(NKUA)
|
3:30 PM
|
BBN constraints in models that alleviate the H0 tension
- Mr
Petros Asimakis
(NTUA)
|
3:40 PM
|
Alleviating H0 tension in Horndeski gravity
- Ms
Maria Petronikolou
(NTUA)
|
3:40 PM
|
The interacting galaxy cluster "El Gordo" a massive blow to LCDM cosmology
- Ms
Elena Asencio
(University of Bonn)
|
3:50 PM
|
Testing robustness of supernovae cosmological parameter inference with Gaussian process
- Mr
Bohdan Bidenko
(University of Groningen)
|
3:50 PM
|
The massless limit and tension in massive gauge theories
- Ms
Anamaria Hell
(LMU Munich)
|
4:00 PM
|
A look beyond ΛCDM theory, phenomenology and observations
- Dr
William Giarè
(Galileo Galilei Institute for theoretical physics)
|
4:00 PM
|
Boltzmann solvers in the era of cosmological tensions: symbolic implementation of extensions in PyCosmo
- Ms
Beatrice Moser
(ETH Zurich)
|
4:10 PM
|
Challenging LCDM and the isotropy of the local Universe with galaxy clusters
- Dr
Konstantinos Migkas
(University of Bonn)
|
4:10 PM
|
Quantifying the S8 tension with the Redshift Space Distortion data set
- Dr
David Benisty
(Ben Gurion U. of Negev)
|
4:20 PM
|
Can intermediate time scales modified gravity theories solve the s8 and H0 tensions ?
- Dr
Ziad Sakr
(IRAP Toulouse)
|
4:20 PM
|
Correlations between galaxy angular momenta and initial conditions
- Dr
Pavel Motloch
(CITA, University of Toronto)
|
4:30 PM
|
Resolving Hubble Tension with New Gravitational Scalar Tensor Theories
- Dr
Shreya Banerjee
(Friedrich Alexander University, Erlangen, Germany)
|
4:30 PM
|
The last 10 billion years of cosmic structure growth
- Mr
Carlos Garcia Garcia
(University of Oxford)
|
4:40 PM
|
Alleviating H0 tension in entropic cosmology
- Dr
Andreas Lymperis
(University of Patras)
|
4:40 PM
|
The H0 tension alleviated through ultra-light primordial black holes: an information insight through gravitational waves
- Dr
Theodoros Papanikolaou
(National Observatory of Athens)
|
4:50 PM
|
A new constraint on Early Dark Energy using the profile likelihood
- Ms
Laura Herold
(Max Planck Institute for Astrophysics, Munich)
|
4:50 PM
|
As good as it gets -- solving the H0-tension à la Ellis & Stoeger
- Dr
Jenny Wagner
|
5:00 PM
|
Can we alleviate the tensions using ANN
- Dr
Konstantinos Dialektopoulos
(Aristotle University of Thessaloniki)
|
5:00 PM
|
Tensions in the deceleration parameter the effect of peculiar velocities in the time-like and null q
- Dr
Jessica Santiago
(Aristotle University of Thessaloniki)
|
5:10 PM
|
Assessing tensions in CMB Polarization data by extending the Minkowski Functional framework
- Mr
Javier Carron Duque
(University of Rome Tor Vergata)
|
5:10 PM
|
Impact of redshift systematics and intrinsic alignment modelling on the S8-tension
- Mr
Silvan Fischbacher
(ETH Zurich)
|
5:20 PM
|
Clustering effects on GWs Dark Sirens determination of Ho A simulations study
- Mr
Marios Kalomenopoulos
(University of Edinburgh)
|
5:20 PM
|
Early dark energy in the light of large scale structure data
- Ms
Rafaela Gsponer
(Institute of Cosmology and Gravitation)
|
5:30 PM
|
--- Coffee break ---
|
6:30 PM
|
Update on GW standard siren cosmology
- Prof.
Daniel Holz
(University of Chicago)
|
7:00 PM
|
Tensions and anomalies: how well do we understand subtle dependencies of galaxy clustering on their properties?
- Prof.
Agnieszka Pollo
(National Center for Nuclear Research)
|
7:20 PM
|
Interacting vacuum and tensions
- Dr
Marco Bruni
(University of Portsmouth)
|
7:40 PM
|
Conference Closure
-
Emmanuel Saridakis
Eleonora Di Valentino
(until 8:00 PM)
|