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The seminar of the Astro & Theory Section takes place Wednesdays  in E??   and on zoomE2-127 (Marie Curie meeting room), starting normally at 14.15. If you would like to suggest a seminar speaker or want to be added to the email list, please contact the organizer (Michael.Kachelriess@ntnu.no).

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  • 27.03., Tor Nordam (SINTEF and IFY NTNU): Transport modelling with stochastic differential equations
    Abstract: Stochastic transport models have existed at least the early 1900s, when Einstein (1905) and Langevin (1908) published two papers with mathematical models for Brownian motion. Einstein described this as a random displacement process, where a particle moves a distance at during each time interval. Langevin, on the other hand, described a random acceleration process, where a particle changes its velocity by a random amount during each time interval. In this talk, I will give a short historical introduction, and then discuss differences and similarities between the two models.

  • 29.03. Jordan Simpson (IFY, NTNU): ??
    Abstract:  On


  • 19.04. Enrico Peretti  (NBI): ??
    Abstract:  I
    slides 

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  • 26.04.,  Mark Kennedy (U Cork):  ??
    Abstract: Co


  • 03.05. Jordan Simpson (IFY, NTNU): Cataclysmic variables with HiPERCAM
    Abstract:  Cataclysmic variables (CVs) are close interacting binary systems consisting of a white dwarf star (primary) accreting matter from a low-mass companion (secondary). As the end-state of many main sequence binaries, and potential progenitors to Type Ia supernovae, CVs form a crucial stage in the evolution of a wide variety of systems. The classical theory of CV evolution has persisted for over 40 years, despite its continuing failures to explain observations. Recently, a new empirical model has emerged that potentially explains many issues in CV evolution - however, a physical basis for this model is still needed. Using the ultra-fast quintuple-band imager HiPERCAM, along with advanced modelling techniques, the team at Sheffield (and collaborators) measures CVs with unprecedented precision to test this new model and ultimately resolve the long-standing problems in CV evolution once and for all.


  • 23.05., Mathias Pavely Noedtvedt (IFY, NTNU): ???                      Abstract:


  • 10.5., Alice Harding (Los Alamos): ??? Abstract:

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