hanse2011.desy.de

HAvSE: HAmburg neutrinos from Supernova Explosions

How to reach DESY. HAvSE: HAmburg neutrinos from Supernova Explosions. HAνSE is a meeting focused on recent progresses and open problems in supernova neutrino physics, ranging from supernova modelling to particle physics aspects and detection strategies. The aim of this meeting is to bring together experts working on various aspects of these phenomena, review the progress in understanding them, and discuss future courses of action. The members of the organizing committee are:. Download the poster as PDF.

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HAvSE: HAmburg neutrinos from Supernova Explosions | hanse2011.desy.de Reviews

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How to reach DESY. HAvSE: HAmburg neutrinos from Supernova Explosions. HAνSE is a meeting focused on recent progresses and open problems in supernova neutrino physics, ranging from supernova modelling to particle physics aspects and detection strategies. The aim of this meeting is to bring together experts working on various aspects of these phenomena, review the progress in understanding them, and discuss future courses of action. The members of the organizing committee are:. Download the poster as PDF.

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1 scientific programme

2 organisation

3 participants

4 talks

5 slides

6 accomodation

7 events

8 pictures

9 proceedings

10 middot;

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HAvSE: HAmburg neutrinos from Supernova Explosions | hanse2011.desy.de Reviews

https://hanse2011.desy.de

How to reach DESY. HAvSE: HAmburg neutrinos from Supernova Explosions. HAνSE is a meeting focused on recent progresses and open problems in supernova neutrino physics, ranging from supernova modelling to particle physics aspects and detection strategies. The aim of this meeting is to bring together experts working on various aspects of these phenomena, review the progress in understanding them, and discuss future courses of action. The members of the organizing committee are:. Download the poster as PDF.

INTERNAL PAGES

hanse2011.desy.de

1

Slides

http://hanse2011.desy.de/e119287

How to reach DESY. Stephan Bruenn: Neutrinos and core-collapse Supernovae. Christian Ott: New Aspects and Boundary Conditions of Core-Collapse Supernova Theory. Bernhard Mueller: Neutrinos and Gravitational Waves from core-collapse supernovae. Rebecca Surman: Neutrinos and Supernova Nucleosynthesis. Almudena Arcones: Neutrino-driven winds and nucleosynthesis of heavy elements. Gang Shen: Equation of State and neutrino signals in supernovae. Tina Lund: Neutrino Signatures of Supernova SASI-now in 3d.

2

How to reach DESY

http://hanse2011.desy.de/e108369

How to reach DESY. How to reach DES. How to reach DESY. How to reach DESY. DESY Hamburg Site, main entrance. To Hamburg Altona station:. Continue by taxi, traveling time approx. 15-20 min. Or continue by bus line 1 (direction Schenefelder Holt) directly to the main entrance of DESY (bus stop Zum Hünengrab/DESY), traveling time approx. 25 min. Or continue by S-Bahn (local city train) line S1 or S11 (direction Blankenese/Wedel) to Othmarschen. Then go on with bus line 1 (direction Schenefelder Holt). Exit ...

3

List of participants

http://hanse2011.desy.de/e109028

How to reach DESY. List of participants updated on 14th July. 2015 Deutsches Elektronen-Synchrotron DESY.

4

HAvSE: HAmburg neutrinos from Supernova Explosions

http://hanse2011.desy.de/index_print_eng.html

URL: index eng.html. HAvSE: HAmburg neutrinos from Supernova Explosions. HAνSE is a meeting focused on recent progresses and open problems in supernova neutrino physics, ranging from supernova modelling to particle physics aspects and detection strategies. The aim of this meeting is to bring together experts working on various aspects of these phenomena, review the progress in understanding them, and discuss future courses of action. The members of the organizing committee are:. Download the poster as PDF.

5

Speakers & Talks

http://hanse2011.desy.de/e112831

How to reach DESY. Baha Balantekin (University of Wisconsin):. SN Neutrino flavor evolution at high density. Stephan Bruenn (Florida Atlantic University):. Neutrinos and core-collapse Supernovae. Gianluigi Fogli (Bari University):. Neutrino oscillations: an exciting scientific adventure. Amol Dighe (TIFR, Mumbai):. Signatures of SN neutrino oscillations. Natalie Jachowicz (Gent University):. Thomas Janka (MPA, Garching):. Rätselhafte Supernovae - den Geheimnissen der grössten. Mark Vagins (IMPU, Tokyo):.

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How to reach DESY. HAvSE: HAmburg neutrinos from Supernova Explosions. HAνSE is a meeting focused on recent progresses and open problems in supernova neutrino physics, ranging from supernova modelling to particle physics aspects and detection strategies. The aim of this meeting is to bring together experts working on various aspects of these phenomena, review the progress in understanding them, and discuss future courses of action. The members of the organizing committee are:. Download the poster as PDF.

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