Frontiers of Cosmology and Astrophyiscs

Lecture log

Academic year 2025/2026
Lecturer Stefano Carniani, Simona Gallerani

Lecture

  • 03 Mar 2026 (2h 00m)

    STEFANO Carniani - Course (teaching activity) - Face to face

    Introduction to extragalactic astrophysics; historical review of the most important results

  • 10 Mar 2026 (2h 00m)

    STEFANO Carniani - Course (teaching activity) - Face to face

    structure formation; linear perturbation theory; spherical collapse theory

  • 17 Mar 2026 (2h 00m)

    STEFANO Carniani - Course (teaching activity) - Face to face

    Virialized dark matter haloes; Press-Schechter formalism and dark matter halo; Experimental programs to observed matter distribution in the Universe

  • 19 Mar 2026 (2h 00m)

    STEFANO Carniani - Course (teaching activity) - Face to face

    Radiative transfer equation; optical depth; emergent intensity; collisional transitions; forbidden and permitted emission lines

  • 20 Mar 2026 (2h 00m)

    STEFANO Carniani - Course (teaching activity) - Face to face

    galaxy formation; shock heating; collapse condition; fragmentation; radiative cooling

  • 26 Mar 2026 (2h 00m)

    STEFANO Carniani - Course (teaching activity) - Face to face

    interstellar medium; molecular clouds; star formation; stellar populations; spectral energy distribution

  • 01 Apr 2026 (2h 00m)

    STEFANO Carniani - Course (teaching activity) - Face to face

    introduction to black holes; supermassive black holes; active galactic nuclei, unified model

  • 02 Apr 2026 (2h 00m)

    STEFANO Carniani - Course (teaching activity) - Face to face

    accretion disk; thin disk model; radiation emitted by active galactic nuclei

  • 07 Apr 2026 (2h 00m)

    STEFANO Carniani - Course (teaching activity) - Face to face

    radiation pressure; galactic outflows; coevolution between black holes and galaxy; AGN in the early universe; little red dots

  • 09 Apr 2026 (2h 00m)

    STEFANO Carniani - Course (teaching activity) - Face to face

    JWST results; overabundance of galaxy at z>10; new theoretical models of galaxy formation