David Blaschke University of Wroclaw. The New Physics of Compact Stars: CompStar
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1 David Blaschke University of Wroclaw The New Physics of Compact Stars: CompStar
2 David Blaschke University of Wroclaw CompStar in a nutshell duration: 5 years (Feb Feb. 2013) 10 ESF participating countries annual budget: 70.5 k expected key activities: science meetings (conferences, schools, workshops) fellowships (short and long term visits)
3 Steering Committee
4 Steering Committee Poland» Polish Academy of Sciences (PAN), Warsaw Italy» Istituto Nazionale di Fisica Nucleare (INFN), Rome Germany» Deutsche Forschungsgemeinschaft (DFG), Bonn Denmark» Forskningsrådet for Natur og Univers (FNU), Copenhagen Spain» Consejo Superior de Investigaciones Cientificas (CSIC), Madrid» Ministerio de Educacion y Ciencia (MEC) France» Centre National de la Recherche Scientifique (CNRS), Paris Slovak Republic» Slovak Research and Development Agency, Bratislava Switzerland Schweizerischer Nationalfonds (SNF), Bern Portugal» Fundação para a Ciência e a Tecnologia, Lisboa United Kingdom» Science & Technology Facilities Council, Swindon
5 Members
6 CompStar members Members
7 Members CompStar members partners in Europe
8 Members CompStar members partners in Europe other ESF members
9 Members CompStar members partners in Europe other ESF members
10 Members & Partners
11 Members & Partners North America
12 Members & Partners North America South America
13 Members & Partners North America Asia & Australia South America
14 Members & Partners North America Asia & Australia South America Africa
15 Scientific Scope CompStar joins three communities
16 Scientific Scope CompStar joins three communities Topics CO CR ME MF PE SN core physics high density nuclear matter crust physics low density nuclear matter Mergers binary neutron stars and GRB s Magnetic Fields strong fields and cooling processes Perturbations Gravitational Waves signals Supernovae collapse the birth of Neutron Stars
17 Finances and Management schools workshops short visits exchange 0 1 2
18 Finances and Management Publication & publicity ESF administration Grants Science meetings SC meetings Matching funds Astrosim schools workshops short visits exchange
19 Finances and Management Publication & publicity ESF administration Grants Science meetings SC meetings Matching funds Astrosim schools workshops short visits exchange
20 CompStar Schools & Workshops Lądek Zdrój 2008 Coimbra 2009 Caen 2010
21 CompStar Schools & Workshops Lądek Zdrój 2008 FR 5% DE 24% IT 12% DK World 2% 6% EU 14% PL 26% UK 4% CH 4% ES 4% 107 Coimbra 2009 DE 21% FR 10% DK 1% Caen 2010 IT 10% PL 12% World 13% EU 7% UK ES 4% 5% CH 2% 84 PT 13% SK 2% DE 14% FR 27% IT 10% PL 11% World 6% EU 9% UK 7% CH 3% 100 PT SK 8% 1% ES 4%
22 CompStar Schools & Workshops Lądek Zdrój 2008 DE 24% FR 5% CH 4% UK ES 4% 5% CH 2% DE 14% FR 27% PL 12% EU 7% ES 4% Caen 2010 IT 10% World 13% PL 26% UK 4% DE 21% FR 10% DK 1% IT 12% DK World 2% 6% EU 14% Coimbra 2009 PT 13% PL 11% World 6% EU 9% PT SK 8% 1% ES 4% CH 3% UK 7% SK 2% IT 10%
23 Science Meetings 2008 Theoretical issues in nuclear astrophysics, Orsay (France) Dense matter in heavy-ion collisions and astrophysics, Dubna (Russia) The modern physics of compact stars, Yerevan (Armenia) Quantum statistical mechanics and field theory, Wroclaw (Poland) 2009 Neutron stars as gravitational wave sources, Rome (Italy) Defining the neutron star crust: x-ray burst, superbursts and giant flares, Santa Fe (USA) Microphysics in computational relativistic astrophysics, Copenhagen (Denmark) Modeling and observation of neutron stars, Meudon (France) 2010 CompStar EoS workshop, Darmstadt (Germany) Physics and astrophysics of neutron stars and black holes, Bremen (Germany) Mode-SNR-PWN workshop, Bordeaux (France)
24 Networking CO CR ME MF PE SN 2008 CO core physics: high density nuclear matter CR crust physics: low density nuclear matter ME Mergers : binary neutron stars and GRB s MF Magnetic Fields: strong fields and cooling processes PE Perturbations: Gravitational Waves signals SN Supernovae collapse: the birth of Neutron Stars
25 Networking CO CR ME MF PE SN CO core physics: high density nuclear matter CR crust physics: low density nuclear matter ME Mergers : binary neutron stars and GRB s MF Magnetic Fields: strong fields and cooling processes PE Perturbations: Gravitational Waves signals SN Supernovae collapse: the birth of Neutron Stars
26 Publications
27 Publications A&A ApJ CQG EPL JPG MNRAS NPA PRC PRD PRL
28 Publications A&A ApJ CQG EPL JPG MNRAS NPA PRC PRD PRL total # papers # authors paper/author authors/paper countries/paper
29 Future Goals ERA in astronuclear physics with new generation of interdisciplinary researchers EoS of dense matter for astrophysical simulations: supernovae, mergers, evolving compact stars Measures PhD & Postdoc exchange between sites with complementary expertise Schools & Workshops task force CompStar-EoS with six conveners for EoS (3) and applications (3)
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