Physics & Astrophysics
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I was appointed as an RCUK Academic Fellow at Keele University in May 2007 and since 2008, I am also a visiting scientist at the www.IPMU.jp , in Tokyo, Japan. Previously I was a Postdoc at the University of Basel in Switzerland (CH). My undergraduate degree (including masters) in Physics was obtained from the EPFL (Federal Institue of Technology in Lausanne, CH) in 1999. In 1999-2000, I did a one-year industrial training with Mitsubishi Electric in Amagasaki (next to Osaka, Japan). I did my PhD at the University of Geneva (CH) in 2004, under the supervision of Profs Maeder and Meynet on the topic: ‘Massive Rotating Stars: the Road to Supernova Explosions’.
With many collaborators (GB, CH, USA, Japan), I study massive stars and related topics like gamma-ray bursts (GRBs), supernovae (SNe) and the origin of elements by performing numerical simulations. Models are being computed at metallicities ranging from solar down to very low metallicities and from the main sequence until the pre-supernova stage. These models are able to predict properties of the star during its evolution (mass, surface composition and position in the HR diagram), long and soft GRB rates coming from single stars and the production of chemical elements in massive stars.
See my personal web page for further information.
Selected Publications
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Journal Articles
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2007. Very low-metallicity massive stars: Pre-SN evolution models and primary nitrogen production. Astronomy and Astrophysics, vol. 461(2), 571-583. doi>
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2005. Stellar evolution with rotation:XIII. Predicted GRB rates at various Z. Astronomy and Astrophysics, vol. 443(2), 581-591. doi>
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2005. Yields of rotating stars at solar metallicity. Astronomy and Astrophysics, vol. 433, 1013-1022. doi>
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2004. Stellar evolution with rotation. XII, Pre-supernova models. Astronomy and Astrophysics, vol. 425(2), 649-670. doi>
Other
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2010. Stellar Evolution in the Upper HR Diagram. HOT AND COOL: BRIDGING GAPS IN MASSIVE-STAR EVOLUTION (vol. 425, pp. 13-22). link>
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2010. Theoretical stellar Delta Y/Delta O in the early Universe. LIGHT ELEMENTS IN THE UNIVERSE (vol. 5, pp. 447-452). link>
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2009. HUNTING FOR THE IMPRINTS OF THE FIRST STARS. XII IAU REGIONAL LATIN AMERICAN MEETING (vol. 35, pp. 207-208). link>
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2008. Were the first stars fast rotators?. FIRST STARS III (vol. 990, pp. 325-329). link>
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2007. Mass loss and very low-metallicity stars. UNSOLVED PROBLEMS IN STELLAR PHYSICS (vol. 948, pp. 397-404). link>
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2006. Evolution of rotating stars at very low metallicity. Stellar Evolution at Low Metallicity: Mass Loss, Explosions, Cosmology (vol. 353, pp. 49-62). link>
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2006. Rotating massive stars @ very low Z: High C & N production. Origin of Matter and Evolution of Galaxies (vol. 847, pp. 71-76). link>
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2006. Stellar evolution of massive stars at very low metallicities (With 10 Figures). In S. Roeser (Ed.). Reviews in Modern Astronomy (vol. 19, p. 101-+).
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2005. Chemical abundances and yields from massive stars. Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis in Honor of David L. Lambert (vol. 336, pp. 79-92). link>
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2005. Effects of rotation on pre-supernova models. 1604-2004: Supernovae as Cosmological Lighthouses (vol. 342, pp. 99-104). link>
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2005. Evolution of the most massive stars. Fate of the Most Massive Stars, Proceedings (vol. 332, pp. 3-13). link>
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2005. Massive rotating stars: Pre-supernova evolution at solar metallicity. 1604-2004: Supernovae as Cosmological Lighthouses (vol. 342, pp. 131-132). link>
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2005. Pre-supernova evolution of rotating massive stars. COSMIC EXPLOSIONS (vol. 99, pp. 209-213). link>
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2004. Dynamical shear instability. STELLAR ROTATION (pp. 510-511). link>
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2003. Stellar yields in CNO from rotating stellar models. CNO IN THE UNIVERSE (vol. 304, pp. 293-301). link>
- SASP lectures on "Molecular Theory" and "Quantum and Astrophysics

