• Non ci sono risultati.

Varying Fundamental Constants and Dynamical Dark Energy Sesto, Val Pusteria (BZ) , 8-13th July 2013

N/A
N/A
Protected

Academic year: 2022

Condividi "Varying Fundamental Constants and Dynamical Dark Energy Sesto, Val Pusteria (BZ) , 8-13th July 2013"

Copied!
4
0
0

Testo completo

(1)

7

Varying Fundamental Constants and Dynamical Dark Energy

Sesto, Val Pusteria (BZ) , 8-13th July 2013

Scientific Organizing Committee Luca Amendola (Heidelberg University), Bruce Bassett (Cape Town University), Enrique Garcia-Berro (UPC, Barcelona), Susana Landau (Buenos Aires University),

Sergey Levshakov (Ioffe Institute, Saint Petersburg), Joao Magueijo (Imperial College, London),

Paolo Molaro (INAF-OATs co-chair) Carlos Martins, (CAUP, Porto, co-chair)

Michael Murphy (Swinburne University, Melburne), Keith Olive (Minnesota University),

Patrick Petitjean (IAP, Paris),

Dieter Reimers (Hamburg University),

Rodger Thompson (Steward Observatory, Arizona), Wim Ubachs (University of Amsterdam),

Jean-Philippe Uzan (IAP, Paris), Elisabeth Vangioni (IAP, Paris),

John Webb (New South Wales University, Sydney) Local Organizing Committee

Gabriella Deconi (Sexten Center for Astrophysics) Gabriella Schiulaz (INAF-OATs)

Sergio Monai (INAF-OATs) Paolo Molaro (INAF-OATs chair)

Luca Carid´a (Sexten Center for Astrophysics)

Sponsorship

National Institute of Astrophysics (INAF) Consortium for Physics of Trieste

Astonomical Observatory of Trieste (INAF-OATs)

(2)

8

FOREWORD

The concept that fundamental physical constants may change over time dates back to Dirac’s Large Number Hypothesis in the late 1930’s and had been a very fertile idea in theoretical physics and cosmology throughout the XX century. Two fundamental constants, the fine-structure con- stant and the proton-to-electron mass ratio, can be effectively probed by means of the study of intervening absorption systems in the spectra of the more distant quasars, Cosmic Microwave Background and Primordial Nucleosynthesis. At present times the detection of their variation throughout space-time is seen as a possible manifestation of the presence of light scalar fields pervading the Universe, the presence of which is foreseen in many cosmological models trying to account for the dark energy.

All this was discussed at the Workshop Varying Fundamental Constants and Dynamical Dark Energy held in Sesto, Val Pusteria (BZ) , on 8-13th July 2013 in the building of the Primary School of Sesto, under the beautiful landscape of the Dolomites.

The workshop was the last of a series of meeting dedicated to this subject which started with the 1983 meeting at the Royal Society organized by W. H. McCrea, M. Rees, and S. Weinberg on The constants of physics. Successively a JENAM meeting took place in Porto in 2002, which was followed by the conferences on Astrophysics, Clocks and Fundamental Constants organized in Bad Honnef in 2003 and 2007. More recently in 2009 a Joint Discussion Are the Fundamental Constants Varying in Space-time?’ was held at the IAU conference in Rio 2009 and in 2010 the JENAM Symposium 2010 From Varying Couplings to Fundamental Physics’ was held in Lisbon. A series of conferences which testifies the growing interest in the field.

We take the opportunity to thank all the participants for their presentations of unique quality and for sharing their most recent results which made the Workshop particularly successful as it is reflected in these proceedings.

We are grateful to the Scientific Organizing Committee for their valuable advice in making the scientific program. The SOC was composed by Luca Amendola, Bruce Bassett, Enrique Garcia-Berro, Susana Landau, Sergey Levshakov, Joao Magueijo, Michael Murphy, Keith Olive, Patrick Petitjean, Dieter Reimers, Rodger Thompson, Wim Ubachs, Jean-Philippe Uzan, Elisabeth Vangioni, John Webb.

A special thank to Gabriella Deconi, better known among the participants as Gabry-one, and Gabriella Schiulaz, the Gabry-two, of the local organizing committee for making the meeting not only scientifically successful but also very enjoyable. We are pleased to acknowledge financial support from the National Institute of Astrophysics (INAF) and from the Consortium for Physics of Trieste. The Sexten Center for Astrophysics and the Sexten Touristic Association are also acknowledged for the warm hospitality.

The Organizing Committee:

Carlos Martins & Paolo Molaro

cover caption: for the cover of this volume we used a slide from Martin Wendt’s talk who took the reverse of the ”Tre Cime di Lavaredo” peaks to mimic QSO’s absorption lines.

(3)

9

Fig. 1.The conference group

(4)

10

Fig. 2.Enjoying the conference dinner

Fig. 3.Enjoying the conference dinner

Fig. 4.During the lectures

Fig. 5.Michael Kozlov and Victor Flanbaum

Fig. 6. Martin Wendt, Hadi Rahmani, Anand Srianand, Sergei Levshakov and Sandro D’Odorico

Fig. 7. Sandro D’Odorico, Paolo Molaro, Micha and Sergei Levshakov, Martin Wendt

Fig. 8.Ewan Cameron and Nissim Kranekar

Fig. 9.Sergei Levshakov

Riferimenti

Documenti correlati

We find that the cur- rent limits on ∆µ/µ place significant constraints on linear equation of state models and on thawing models where w deviates from −1 at late times.. They

We review the variety of new singularities in homogeneous and isotropic FRW cosmology which differ from standard Big-Bang and Big-Crunch singularities and suggest how the nature

Subsequent observations (2011- 2013) at the Effelsberg 100-m telescope of a sample of eight molecular cores from the Milky Way disk reveal systematic errors in the measured

Importantly, these measurements can also be used to obtain constraints on certain classes of unification scenarios, and we com- pare the constraints obtained for PKS1413+135 with

In addition to the CMB data, in the future a new and larger galaxy surveys will provide new galaxy weak lensing mea- surements that, when combined with Planck, will drastically

However, and despite the fact that tests of the stability of fundamental couplings are one of the key science drivers for future high- resolution ultra-stable spectrographs such

We illustrated the abilities of HIRES to probe the nature of Dark Energy in the otherwise un- explored redshift range 2 < z < 5.The results also show that being able

to model the physical systems used to set the constraints (and to determine the effective parameters that can be observationally con- strained to a set of fundamental constants);