Conférences - Astronomie, astrophysique et cosmologie - Italie

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1.
 
Sweeping galaxies clean: cold molecular outflows as drivers of galaxy evolution
ID
719431
Date de début
15 fév 2016
Lieu
Sexten Center for Astrophysics, Italie
2.
 
Rencontres de Physique de La Thuile — XXX Rencontres de Physique de La Vallee d'Aoste
ID
734705
Dates
06 mar 2016 - 12 mar 2016
Lieu
La Thuile, Italie
Sujets
Particle Physics Theoretical ; Particle Physics Phenomenology ; Astroparticle Physics
3.
 
Moriond Cosmology 2016 — 51st Rencontres de Moriond on Cosmology
ID
772304
Dates
19 mar 2016 - 26 mar 2016
Lieu
La Thuile, Italie
Sujets
Cosmic Microwave Background ; Dark Energy ; Clusters ; SZ ; Dark Matter ; Neutrino cosmology ; inflation ; massive gravity ; spectral distorsions ; 21 cm
4.
 
MODEST 16 — COSMIC-LAB: Star Clusters as Cosmic Laboratories for Astrophysics, Dynamics and Fundamental Physics
ID
787300
Dates
18 avr 2016 - 22 avr 2016
Lieu
Bologna, Italie
Résumé
Cosmic-Lab is a five-year project aimed at probing the complex interplay between dynamics and stellar evolution by using Galactic globular clusters as cosmic laboratories, and the most exotic by-products of this interplay (blue straggler stars, millisecond pulsars, and intermeditae-mass black holes) as test-particles. The project has been funded by the European Research Council (ERC), within the 2010 Advanced Grant call. The Principal Investigator is Francesco R. Ferraro of the Physics and Astronomy Department of the University of Bologna. The project will end on 2016 April 30th and this international conference is meant to be its final action. The purpose of the conference is to put together theorists and observers for discussings the status of the research on the COSMIC-LAB topics. Accordingly, the conference is organized in four main sections: blue straggler stars (BSSs), millisecond pulsars (MSPs), intermediate-mass black holes (IMBHs) and dynamics of collisional systems (Dyn).
Contact
Francesco R. Ferraro;     Tél.: [+390512095774];     Email.: francesco.ferraro3@unibo.it
Sujets
globular clusters, dynamics, exotic stellar populations
5.
 
CSQCD V — Compact Stars in the QCD phase diagram V
ID
786920
Dates
23 mai 2016 - 27 mai 2016
Lieu
L'Aquila, Italie
Résumé
The aim of this Conference is to bring together physicists working on strong interacting dense matter, QCD phase diagram, ultrarelativistic heavy-ion collisions with astrophysicists working on Compact Stars (from their birth in core-collapse supernovae to their old age as cold radio pulsars including binary merger events) and on related phenomena. A profound theoretical description of these phenomena necessarily involves the equation of state and transport properties of QCD matter that are derived from nonperturbative quantum field theories, many-body physics of strong interacting matter and phenomenological investigations.

The CSQCD conference will take place at the Gran Sasso Science Institute (GSSI) in L'Aquila (Italy). GSSI is an international PhD school and a center for research and higher education. On May 25 the CSQCD conference will take place at the Gran Sasso National Laboratories (LNGS). LNGS is one of the four national laboratories of INFN (National Institute for Nuclear Physics). It is the largest underground laboratory in the world for experiments in particle physics, particle astrophysics and nuclear astrophysics. Participants to the conference will be picked up at the hotels and transported to LNGS. An underground guided tour will take place that day.

Contact
Ignazio Bombaci;     Email.: compact.stars@lngs.infn.it
Sujets
Equation of state and QCD phase transitions, QCD in astrophysics of compact stellar objects, supernovae and compact stars mergers, Strangeness in Compact Stars, Strange Stars, Hadron production in heavy-ion collisions, Nonequilibrium and transport phenomena in dense matter.
6.
 
Summer School on Energy “Giacomo Ciamician”
ID
772055
Dates
27 jui 2016 - 01 jul 2016
Lieu
Sexten Centre for Astrophysics, Sexten (Sesto), Italie
7.
 
BAO & RSD: dark light on obscure acronyms
ID
772054
Dates
04 jul 2016 - 08 jul 2016
Lieu
Sexten Centre for Astrophysics, Sexten (Sesto), Italie
8.
 
Theoretical challenges for precision galaxy clustering
ID
772108
Dates
11 jul 2016 - 15 jul 2016
Lieu
Sexten Centre for Astrophysics, Sexten (Sesto), Italie
9.
 
Industrial Revolution in Galactic Astronomy
ID
772074
Dates
18 jul 2016 - 22 jul 2016
Lieu
Sexten Centre for Astrophysics, Sexten (Sesto), Italie
10.
 
The Role of Feedback in the Formation and Evolution of Star Clusters
ID
772139
Dates
18 jul 2016 - 22 jul 2016
Lieu
Sexten Centre for Astrophysics, Sexten (Sesto), Italie
11.
 
Summer School J.S. Bell on Quantum Mechanics
ID
772094
Dates
25 jul 2016 - 29 jul 2016
Lieu
Sexten Centre for Astrophysics, Sexten (Sesto), Italie
12.
 
Multiple Populations in Stellar Clusters: Where do we stand?
ID
772137
Dates
25 jul 2016 - 29 jul 2016
Lieu
Sexten Centre for Astrophysics, Sexten (Sesto), Italie
13.
 
Invisibles 2016 Workshop
ID
787486
Dates
12 sep 2016 - 16 sep 2016
Lieu
Padova, Italie
Résumé
Invisibles 16 is the fifth thematic workshop organised in the context of the H2020 funded ELUSIVES ITN (H2020-MSCA-ITN-2015, GA-2015-674896-ELUSIVES) and InvisiblesPlus (H2020-MSCA-RISE-2015, GA-2015-690575-InvisiblesPlus) which focuses on Neutrino, Dark Matter and Dark Energy phenomenology and their connection, and more generally on physics beyond the Standard Model of Particle Physics.
Contact
Email.: inv16workshop@pd.infn.it
Sujets
High Energy Physics, Neutrinos, Dark Matter, Dark Energy, Higgs.
14.
 
Breaking the Limits: Super-Eddington Accretion on Compact Objects
ID
771847
Date de début
19 sep 2016
Lieu
Arbatax (OG), Sardinia, Italie
15.
 
VIALACTEA 2016 — The Milky Way as a Star Formation Engine: Towards a predictive Galaxy-scale model of the Star Formation Life-Cycle
ID
770255
Dates
26 sep 2016 - 30 sep 2016
Lieu
Rome, Italie
Résumé
The Milky Way Galaxy is a complex ecosystem where a cyclical transformation process brings diffuse baryonic matter into dense unstable condensations to form stars. Although considerable progress has been made in the last two decades in the understanding of the evolution of isolated dense molecular clumps toward the onset of gravitational collapse and the formation of stars and planetary systems, several key-questions remain elusive. The creation of a fundamental theory or, rather, of a galaxy-scale predictive model for star formation, is a key challenge. We enter a new era where a new suite of cutting-edge Milky Way surveys of the entire Galactic Plane have already started to transform the view of our Galaxy as a global star formation engine. The combination of near-IR ground surveys data, mid-IR and far-IR dust continuum obtained by ESA's HERSCHEL and NASA's SPITZER and WISE satellites, submillimeter and radio continuum, and gas-tracing atomic and molecular spectroscopy from ground-based antennas, is for the first time unlocking access to angular scales below 30" across 4 decades in wavelength for both the dust and the three gas components of the ISM (molecular, atomic and ionised). The integrated science analysis of these massive and diverse datasets requires new concepts of 3D-based visual analytics tools that integrate data access, sources and features extraction, model fitting and source classifications.
Contact
Sergio Molinari;     Email.: vialactea2016@iaps.inaf.it
Sujets
From the diffuse texture of the ISM to the backbone skeleton of the Milky Way, Demographics of Galactic Clumps and Cluster Progenitors, Triggering, Spiral Arms, Turbulence and Gravitation, The 3-D Galaxy from the near-infrared to the radio, The Milky Way in the context of nearby galaxies and of extra-galactic star formation recipes, Visual analytics, data mining and science gateways
16.
 
IAU Symposia: Astroinformatics
ID
761927
Dates
29 sep 2016 - 04 oct 2016
Lieu
Sorrento, Italie
Résumé
The proposed symposium will bring together world-class experts to address the methodological and technological challenges posed by massive data sets produced by the new generation of telescopes and observatories. Astronomy is at the forefront of Big Data science with exponentially growing data volumes and data rates, now entering the petascale regime at optical, infrared and radio wavelengths. The data structures are not simple, and the procedures for using them to gain astrophysical insights are not obvious. Astronomy is truly becoming data-driven in the ways that are both quantitatively and qualitatively different from the past. The informational content of the modern data sets is so high that archival research and data mining not merely profitable, but practically obligatory; researchers who obtain the data can only extract a small fraction of the science that is enabled by it.
17.
 
Astronomical Data Analysis Software and Systems (ADASS) XXVI
ID
780720
Date de début
16 oct 2016
Lieu
Trieste, Italie
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Dernière mise à jour: 27 Janvier 2016