David Blaschke University of Wroclaw The New Physics of Compact Stars: CompStar
David Blaschke University of Wroclaw CompStar in a nutshell duration: 5 years (Feb. 2008 - 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)
Steering Committee
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
Members
CompStar members Members
Members CompStar members partners in Europe
Members CompStar members partners in Europe other ESF members
Members CompStar members partners in Europe other ESF members
Members & Partners
Members & Partners North America
Members & Partners North America South America
Members & Partners North America Asia & Australia South America
Members & Partners North America Asia & Australia South America Africa
Scientific Scope CompStar joins three communities
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
Finances and Management 2008 2009 2010 schools 2 1 1 workshops 4 4 4 short visits 1 5 3 exchange 0 1 2
Finances and Management Publication & publicity ESF administration Grants Science meetings SC meetings Matching funds Astrosim 2008 2009 2010 schools 2 1 1 workshops 4 4 4 short visits 1 5 3 exchange 0 1 2 120000 100000 80000 60000 40000 20000 0 2008 2009 2010
Finances and Management Publication & publicity ESF administration Grants Science meetings SC meetings Matching funds Astrosim 2008 2009 2010 schools 2 1 1 workshops 4 4 4 short visits 1 5 3 exchange 0 1 2 120000 100000 80000 60000 40000 20000 0 2008 2009 2010
CompStar Schools & Workshops Lądek Zdrój 2008 Coimbra 2009 Caen 2010
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%
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% 100 84 107 CH 3% UK 7% SK 2% IT 10% 87 90 85 67 60 30 14 2008 6 6 2009 11 9 2010 6 0
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)
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
Networking CO CR ME MF PE SN 2010 2009 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
Publications
Publications A&A ApJ CQG EPL JPG MNRAS NPA PRC PRD PRL 0 5 10 15 20 25
Publications A&A ApJ CQG EPL JPG MNRAS NPA PRC PRD PRL 0 5 10 15 20 25 total 2008 2009 2010 # papers 113 25 43 45 # authors 149 41 81 88 paper/author 2.1 1.3 1.6 1.5 authors/paper 3.7 4.0 3.7 3.4 countries/paper 2.3 2.6 2.3 2.2
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) www.compstar-esf.org