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The time is ripe for a critical assessment of our present knowledge of quasars as accreting black holes and of their evolution across the cosmic time. The aim of this meeting is to review and contextualize the main observational scenarios following an empirical approach, to present and discuss the accretion scenario, and then to analyze how a closer connection between theory and observation can be achieved, identifying those aspects of our understanding that are still on a shaky terrain and are therefore uncertain knowledge.
Theoretical models and numerical simulations have been developed in order to capture the complexity of this interaction and to understand when, where, and how feedback takes place. At the same time the ICM is an important diagnostic of the dynamics of the cluster itself, and an exhaustive understanding of its properties is crucial for a full understanding of the growth of cosmic structures at large, and the measurement of cosmological parameters. This workshop will focus on the physics of the ICM and its relation with the different mass components of galaxy clusters. The aim is to provide an overview of the many exciting recent results at vastly different wavelengths (Radio, SZ, sub-mm, IR, optical, X-ray, gamma-ray) and use them to challenge theoretical models and advanced numerical simulations.
The meeting will take place at the University of Sheffield, in the new Diamond facility. It will start on Monday 10th April. Following the end of the conference on Wednesday 12th April, there will be an STFC town hall and then a public lecture.
To fully realise the potential of the SKA as a machine for fundamental physics, the SKA organisation seeks to engage the theoretical physics community in the science case and design considerations for the full array. To initiate this discussion, we will be holding a focused workshop in May 2017, in which we aim to bring together radio astronomers and theorists to jointly consider ways in which the SKA can test and explore fundamental physics.
STARS2017 – New phenomena and new states of matter in the Universe, general relativity, gravitation, cosmology, heavy ion collisions and the formation of the quark-gluon plasma, white dwarfs, neutron stars and pulsars, black holes, gamma-ray emission in the Universe, high energy cosmic rays, gravitational waves, dark energy and dark matter, strange matter and strange stars, antimatter in the Universe, and topics related to these.
SMFNS2017 – Strong magnetic fields in the Universe, strong magnetic fields in compact stars and in galaxies, ultra-strong magnetic fields in neutron star mergers, quark stars and magnetars, strong magnetic fields and the cosmic microwave background, and topics related to these.
The meeting will place GC systems in the context of their host galaxy and the interplay between them.
The school will host 40 graduate students and young researchers from all over the globe, and is designed to be very interactive with ample time for questions and discussions. During the two weeks of the TSI, the afternoons will be dedicated to hands-on problem solving to help digest the content of the lectures. TSI 2017 is designed to be accessible to students working in nuclear physics and nuclear astrophysics, providing them with a solid foundation in modern methods and tools in all three areas of research, as well as our current understanding of the astrophysical events under study.
The Workshop on Astrophysical Opacities (WAO) intends to gather opacity data producers and consumers from both the atomic and molecular sectors in order to contribute to solving outstanding problems and to develop more effective and integrated interfaces. The last time such a workshop took place was at the IBM Venezuela Scientific Center, Caracas, Venezuela, in July 1991. Taken into consideration the success of this first WAO and the huge scientific advancements that have taken place since then in most related research fields, we have been encouraged to organize a second event. The present WAO will be held at Western Michigan University in the very welcoming town of Kalamazoo, Michigan, USA, where everything good is easily within reach. Contributed papers and student participation is specially encouraged.
A preliminary list of the topics to be developed during the Conference is given below: Nuclear double beta decays; Nuclear structure in connection with neutrino physics; Nuclear reactions as a probe for weak decays; Neutrino-nucleus interaction at low and high energy; Supernova models and detection of supernova neutrinos; Solar models and detection of solar neutrinos; Direct and indirect dark-matter searches; Rare beta decays of nuclei for neutrino-mass measurements; Neutrino oscillations and matter effects; Anomalies in reactor neutrinos; New related detection technologies
Stand vom 27. März 2017