Items where Author is "Hirschi, R."

Article

Nishimura, N. and Rauscher, T. and Hirschi, R. and Cescutti, G. and Murphy, A. St. J. and Frohlich, C.. (2019) Uncertainties in nu p-process nucleosynthesis from Monte Carlo variation of reaction rates. Monthly Notices of the Royal Astronomical Society, 489 (1). pp. 1379-1396.

Rauscher, T. and Nishimura, N. and Cescutti, G. and Hirschi, R. and Murphy, A. St. J.. (2018) Abundance Uncertainties Obtained With the PIZBUIN Framework For Monte Carlo Reaction Rate Variations. AIP Conference Proceedings, 1947. 020015.

Cescutti, G. and Hirschi, R. and Nishimura, N. and den Hartogh, J. W. and Rauscher, T. and Murphy, A. St. J. and Cristallo, S.. (2018) Uncertainties in s-process nucleosynthesis in low-mass stars determined from Monte Carlo variations. Monthly Notices of the Royal Astronomical Society, 478 (3). pp. 4101-4127.

Nishimura, N. and Rauscher, T. and Hirschi, R. and Murphy, A. St J. and Cescutti, G. and Travaglio, C.. (2018) Uncertainties in the production of p nuclides in thermonuclear supernovae determined by Monte Carlo variations. Monthly Notices of the Royal Astronomical Society, 474 (3). pp. 3133-3139.

Cescutti, G. and Nishimura, N. and Hirschi, R. and Rauscher, T. and den Hartogh, J. W. and Murphy, A. S. J.. (2017) The s-process nucleosynthesis: impact of the uncertainties in the nuclear physics determined by Monte Carlo variations. Memorie della Societa Astronomica Italiana, 88 (3). p. 432.

Nishimura, N. and Hirschi, R. and Rauscher, T. and Murphy, A. St. J. and Cescutti, G.. (2017) Uncertainties in s-process nucleosynthesis in massive stars determined by Monte Carlo variations. Monthly Notices of the Royal Astronomical Society, 469 (2). pp. 1752-1767.

Battino, U. and Pignatari, M. and Ritter, C. and Herwig, F. and Denisenkov, P. and Den Hartogh, J. W. and Trappitsch, R. and Hirschi, R. and Freytag, B. and Thielemann, F. and Paxton, B.. (2016) Application of a Theory and Simulation-based Convective Boundary Mixing Model for AGB Star Evolution and Nucleosynthesis. Astrophysical Journal, 827 (1). p. 30.

Rauscher, T. and Nishimura, N. and Hirschi, R.. (2016) Theory considerations for nucleosynthesis beyond Fe with special emphasis on p-nuclei in massive stars. AIP Conference Proceedings, 1743. 040008.

Rauscher, T. and Nishimura, N. and Hirschi, R. and Cescutti, G. and Murphy, A. St. J. and Heger, A.. (2016) Uncertainties in the production of p nuclei in massive stars obtained from Monte Carlo variations. Monthly Notices of the Royal Astronomical Society, 463 (4). pp. 4153-4166.

Pignatari, M. and Zinner, E. and Hoppe, P. and Jordan, C. J. and Gibson, B. K. and Trappitsch, R. and Herwig, F. and Fryer, C. and Hirschi, R. and Timmes, F. X.. (2015) Carbon-rich presolar grains from massive stars. Subsolar 12C/13C and 14N/15N ratios and the mystery of 15N. The Astrophysical Journal Letters, 808 (2). L43.

Jones, S. and Hirschi, R. and Pignatari, M. and Heger, A. and Georgy, C. and Nishimura, N. and Fryer, C. and Herwig, F.. (2015) Code dependencies of pre-supernova evolution and nucleosynthesis in massive stars: Evolution to the end of core helium burning. Monthly Notices of the Royal Astronomical Society (MNRAS), 447 (4). pp. 3115-3129.

Barbuy, B. and Chiappini, C. and Cantelli, E. and Depagne, E. and Pignatari, M. and Hirschi, R. and Cescutti, G. and Ortolani, S. and Hill, V. and Zoccali, M. and Minniti, D. and Trevisan, M. and Bica, E. and Gomez, A.. (2014) High-resolution abundance analysis of red giants in the globular cluster NGC 6522. Astronomy & astrophysics, Vol. 570 , A76.

Nishimura, N. and Hirschi, R. and Pignatari, M. and Herwig, F. and Beard, M. and Imbriani, G. and Goerres, J. and deBoer, R. J. and Wiescher, M.. (2014) Impact of the uncertainty in alpha-captures on Ne-22 on the weak s-process in massive stars. The 12th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG), Vol. 1594. pp. 146-151.

Pignatari, M. and Wiescher, M. and Timmes, F. X. and de Boer, R. J. and Fryer, C. and Heger, A. and Herwig, F. and Hirschi, R.. (2013) Production of carbon-rich presolar grains from massive stars. The astrophysical journal. Part 2, Letters, Vol. 767, H. 2. p. 22.

Pignatari, M. and Zinner, E. and Bertolli, M. G. and Trappitsch, R. and Hoppe, P. and Rauscher, T. and Fryer, C. and Herwig, F. and Hirschi, R. and Timmes, F. X. and Thielemann, F. -K.. (2013) Silicon Carbide Grains of Type C Provide Evidence for the Production of the Unstable Isotope 32Si in Supernovae. The astrophysical journal. Part 2, Letters, Vol. 771, H. 1. p. 7.

Pignatari, M. and Hirschi, R. and Wiescher, M. and Gallino, R. and Bennett, M. and Beard, M. and Fryer, C. and Herwig, F. and Rockefeller, G. and Timmes, F. X.. (2013) The 12C + 12C Reaction and the Impact on Nucleosynthesis in Massive Stars. The astrophysical journal. Part 1, Vol. 762. p. 31.

Hirschi, R. and Frischknecht, U. and Thielemann, F. -K.. (2012) Chemical signature of GRB progenitors at low metallicities. Memorie della Societa Astronomica Italiana Supplementi, Vol. 21. p. 28.

Frischknecht, U. and Hirschi, R. and Thielemann, F. -K.. (2012) Non-standard s-process in low metallicity massive rotating stars. Astronomy & astrophysics, Vol. 538 , L2.

Bennett, M. E. and Hirschi, R. and Pignatari, M. and Diehl, S. and Fryer, C. and Herwig, F. and Hungerford, A. and Nomoto, K. and Rockefeller, G. and Timmes, F. X. and Wiescher, M.. (2012) The effect of 12C +12C rate uncertainties on the evolution and nucleosynthesis of massive stars. Monthly notices of the Royal Astronomical Society, Vol. 420, H. 4, S. 3047–3070.

Frischknecht, U. and Hirschi, R. and Rauscher, T. and Thielemann, F.-K.. (2011) Impact of rotation on the weak s-process. Proceedings of Science, NIC XI , 189.

Frischknecht, U. and Hirschi, R. and Meynet, G. and Ekström, S. and Georgy, C. and Rauscher, T. and Winteler, C. and Thielemann, F.-K.. (2010) Constraints on rotational mixing from surface evolution of light elements in massive stars. Astronomy & astrophysics, Vol. 522 , A39.

Thielemann, F. K. and Argast, D. and Brachwitz, F. and Fisker, J. L. and Frohlich, C. and Hirschi, R. and Kolbe, E. and Mocelj, D. and Rauscher, T.. (2005) Nuclear physics : a key ingredient in astrophysical modeling. Nuclear physics. A, Nuclear and hadronic physics, Vol. 751 , S. 301C-326C.

Conference or Workshop Item

Nishimura, N. and Hirschi, R. and Rauscher, T.. (2018) Sensitivity to neutron captures and beta-decays of the enhanced s-process in rotating massive stars at low metallicities. In: Journal of Physics: Conference Series, 940.

Nishimura, N. and Cescutti, G. and Hirschi, R. and Rauscher, T. and Den Hartogh, J. and Murphy, A. S. J.. (2017) Impacts of Nuclear-Physics Uncertainty in Stellar Temperatures on the s-Process Nucleosynthesis. In: Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016), 14. 020903.

Rauscher, T. and Nishimura, N. and Hirschi, R. and Cescutti, G. and Murphy, A. S. J. and Heger, A.. (2017) Production Uncertainties of p-Nuclei in the γ-Process in Massive Stars Using a Monte Carlo Approach. In: Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016), 14. 010509.

Frischknecht, U. and Hirschi, R. and Meynet, G. and Ekström, S. and Georgy, C. and Rauscher, T. and Winteler, C. and Thielemann, F.-K.. (2010) Boron depletion in 9 to 15 M_sol stars with rotation. In: Light Elements in the Universe. Cambridge University Press, pp. 421-422.

Thielemann, F. -K. and Fröhlich, C. and Hirschi, R. and Liebendoerfer, M. and Dillmann, I. and Mocelj, D. and Rauscher, T. and Martinez-Pinedo, G. and Langanke, K. and Farouqi, K. and Kratz, K. -L. and Pfeiffer, B. and Panov, I. and Nadyozhin, D. K. and Blinnikov, S. and Bravo, E. and Hix, W. R. and Hoflich, P. and Zinner, N. T.. (2007) Production of intermediate-mass and heavy nuclei. In: Progress in particle and nuclear physics, Vol. 59, No. 1. Oxford, pp. 74-93.