26 August 2024 to 4 September 2024
Orthodox Academy of Crete, Kolymbari, Crete, Greece
Europe/Athens timezone
The extended day of ICNFP 2024 will be 12 December 2024: https://indico.cern.ch/event/1486482/

Session

Workshop on Astro-Cosmo-Gravity

26 Aug 2024, 09:30
Orthodox Academy of Crete, Kolymbari, Crete, Greece

Orthodox Academy of Crete, Kolymbari, Crete, Greece

Conveners

Workshop on Astro-Cosmo-Gravity

  • Alexander Dolgov

Workshop on Astro-Cosmo-Gravity

  • Armen Sedrakian

Workshop on Astro-Cosmo-Gravity

  • Armen Sedrakian

Workshop on Astro-Cosmo-Gravity

  • Armen Sedrakian

Presentation materials

There are no materials yet.

  1. Prof. Armen Sedrakian
    26/08/2024, 09:30
    Workshop on Astro-Cosmo-Gravity
    Talk

    Relativistic density functionals based on baryon-meson Lagrangians can
    be used to describe effectively dense matter in compact stars
    including hyperonic and Delta-resonance degrees of
    freedom. These can be supplemented with a first-order phase transition
    to quark matter at high densities to describe hybrid compact stars.
    I will discuss how the mass-radius and tidal deformability...

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  2. Dr Andrey Alexandrov (University Federico II and INFN, Naples (IT))
    26/08/2024, 12:20
    Workshop on Astro-Cosmo-Gravity
    Talk

    The nature of dark matter is one of the most relevant open problems both in cosmology and particle physics. Many different experimental techniques have been designed and built to detect Weakly Interactive Massive Particles (WIMPs) as dark matter candidates via their scattering with detector atoms. The NEWSdm experiment, located in the Gran Sasso underground laboratory in Italy, is based on a...

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  3. Prof. Francesco Longo (University of Trieste and INFN, Trieste)
    26/08/2024, 12:40
    Workshop on Astro-Cosmo-Gravity
    Talk

    The Cherenkov Telescope Array Observatory (CTAO) will be the next-generation ground-based gamma-ray observatory. CTAO is an array of Imaging Cherenkov Telescopes (IACTs) with sites in the northern and southern hemispheres covering the entire sky. Spanning the energy range from 20 GeV to 300 TeV and offering sensitivity one order of magnitude better than current-generation Imaging Cherenkov...

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  4. David Blaschke
    28/08/2024, 09:00
    Workshop on Astro-Cosmo-Gravity
    Talk

    We explore the conditions under which a first-order deconfinement phase transition in cold and warm neutron star cores would lead to the formation of a third family of compact stars and thus to cold and thermal twin stars. When this transition occurs in a low-mass X-ray binary system, possibly coupled with secondary kick mechanisms such as neutrino or electromagnetic rocket effects, it may...

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  5. Prof. Madhukar Mishra (Department of Physics, Birla Institute of Technology and Science, Pilani, Pilani Campus)
    28/08/2024, 11:20
    Workshop on Astro-Cosmo-Gravity
    Talk

    , We employ here the modified system of Tolman–Oppenheimer–Volkoff (TOV) equations due to the presence of a magnetic field to study the emission properties of the strongly magnetized neutron stars (NSs). We have considered the distance-dependent magnetic field in the modified TOV system of equations. We used three different equations of states (EoSs), namely APR, FPS, and SLY to solve these...

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