Below is the suggested schedule of talks for the first meeting of the new team. The basic format I propose is to have\u00a0talks in the morning and then discussions (in smaller groups if required) in the afternoons.\u00a0This is not meant to be overly prescriptive, and the schedule can be varied as required by the group.<\/p>\n
Talk titles link to the abstracts page<\/a> (where available).<\/p>\n On Monday\u00a0I would like to request summary talks\u00a0to set the stage and context, presenting the state of knowledge in different aspects (simulations, observations, nuclear experiment etc.). Each day Tuesday\u2013Thursday will then be devoted to one of these areas.<\/p>\n For those who are not yet represented in the schedule, please feel free to add your own talk topics to the section of choice<\/p>\n Monday \u2013 introduction<\/strong><\/p>\n M. Falanga \u2013 welcome and introduction to ISSI<\/p>\n D. Galloway \u2013 team logistics, goals, and approach of the workshop<\/p>\n H. Schatz \u2013 status\u00a0of nuclear experiments relevant to thermonuclear bursts (TBC)<\/p>\n D. Galloway \u2013 status of burst observations<\/p>\n 1700h\u00a0\u2013 welcome reception @ ISSI<\/em><\/p>\n Tuesday \u2013 simulations<\/strong><\/p>\n A. Heger \u2013 status of burst modelling<\/p>\n J. Lattimer \u2013 Summary of neutron star radius from observations, theory and experiment with implications for the core-crust interface including pasta<\/p>\n A. Cumming \u2013 Kepler simulations for GS 1826-24<\/p>\n F. Theielmann \u2013\u00a0Spherical Simulations of Multple X-ray Bursts: Aiming for Superbursts<\/p>\n Wednesday \u2013 observations<\/strong><\/p>\n A. Deibel \u2013\u00a0The \u201canomalous” shallow heating mechanism in neutron star transients<\/a><\/p>\n J. Chenevez \u2013 burst observations with\u00a0NuSTAR and the 2014 soft state of GS 1826-24<\/p>\n L. Keek \u2013\u00a0Anisotropic Reflection of Carbon Flames<\/a><\/p>\n Thursday \u2013 nuclear\u00a0experiment & modelling<\/strong><\/p>\n H. Schatz \u2013 sensitivity of burst simulations to nuclear rate uncertainties<\/p>\n Y. Sun \u2013\u00a0Shell models for nuclei in the rp<\/em>-process<\/a><\/p>\n W. Misch \u2013 Electron capture and nuclear de-excitation in silicon burning<\/p>\n Z. Meisel \u2013\u00a0Urca\u00a0cooling prospects for model inputs by\u00a0future nuclear experiments<\/p>\n Friday \u2013 additional\u00a0topics<\/strong><\/p>\n W. Ong \u2013\u00a0Potential bypass of the 56<\/sup>Ni waiting point<\/p>\n A. Cumming \u2013 chemical separation in accreting neutron stars<\/p>\n A. Deibel \u2013\u00a0Shallow Urca cooling pairs in the accreted neutron star ocean and crust<\/a><\/p>\n J. Chenevez \u2013 The NICER mission: capabilities, status, and expectations for burst science<\/a><\/p>\n <\/p>\n","protected":false},"excerpt":{"rendered":" Below is the suggested schedule of talks for the first meeting of the new team. The basic format I propose is to have\u00a0talks in the morning and then discussions (in smaller groups if required) in the afternoons.\u00a0This is not meant … Continue reading