Сессия

Afternoon session 4

4
25 нояб. 2026 г., 14:30

Описание

Afternoon session (November 25)

Presentation materials

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  1. Dmitry Gorbunov (INR RAS)
    25.11.2026, 14:30
  2. YIFU CAI (University of Science and Technology of China)
    25.11.2026, 15:15

    Abstract
    Astonishingly, it was discovered that distant Type Ia supernovae (SN Ia) were accelerating away at an increasing pace. This led to the great discovery of late-time cosmic acceleration and brought us the concept of dark energy, responsible for such a phenomenon. However, the underlying nature remains mysterious. Theoretically, modified gravity can be a framework to provide an...

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  3. Cristhian Garcia Quintero (Center for Astrophysics Harvard-Smithsonian)
    25.11.2026, 16:15

    Abstract
    Current discrepancies between datasets analyzed in the standard model open the possibility for beyond-LCDM model physics, such as evolving dark energy. However, departures from the standard theory of gravity itself can be potentially misinterpreted as dark energy. Fortunately, the growth of galaxy clustering data provides a way to distinguish between the two. In this talk, we...

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  4. Julio Cesar Fabris (Universidade Federal do Espírito Santo)
    25.11.2026, 17:00

    Abstract
    The standard cosmological model has been successful in describing the ob- served universe. It is a simple model that reproduces different observational data using only a few components of matter and energy. It is based on the Theory of General Relativity. However, this success is achieved by introducing a dark sector composed of dark matter and dark energy, components not yet di-...

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  5. Hermano Velten (Universidade Federal de Ouro Preto)
    25.11.2026, 17:45

    Abstract
    We review nonconservative theories of gravity with particular attention to f(R,T) theories (where T is the trace of the energy-momentum). We provide astrophysical and cosmological consequences of a nonvanishing four-divergence of the energy-momentum tensor.
    Links
    https://doi.org/10.3390/universe7020038 10.1016/j.dark.2023.101401

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  6. 25.11.2026, 18:30

    Discussion leader: Dmitry Gorbunov (INR RAS, Moscow)

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