Conveners
Morning session: Dark Matter Galactic Center
- Carlo Luciano Bianco (ICRANet)
Morning session: Dark Matter Galactic Center
- Aldo Treves (Università Insubria)
Morning session: Dark Matter Galactic Center
- Piero Rosati ()
Morning session: AGNs
- Gregory Vereshchagin (ICRANet)
Morning session: Fronteer
- She-Sheng Xue (ICRANet, Physics Department, Sapienza University of Rome)
Morning session: Cocoon and BdHN model
- Yerlan Aimuratov (Fesenkov Astrophysical Institute / al-Farabi Kazakh National University)
Morning session: Cocoon and BdHN Model
- Liang Li (ICRANet, Piazza della Repubblica 10, I-65122 Pescara, Italy)
Morning session: Supernovae
- Maria Dainotti (National Astronomical Observatory of Japan)
Morning session: GRB 171205A and GRB 220101
- Carlos Raúl Argüelles (Universidad Nacional de La Plata)
I will review the use of the Intergalactic Medium as a probe of fundamental physics.
Pioneered with the Christodoulou-Ruffini irreducible mass and subsequently reformulated with the Hawking-Bekenstein entropy, it can be shown that the area of the horizon of a black hole cannot decrease. Partly motivated by the arrow of time problem in cosmology and the Weyl curvature hypothesis, previous works in the literature have proposed - among other possibilities - the square of the...
The recent high-precision measurement of the $W$ mass by the CDF collaboration is in $7.0~\sigma$ tension with the Standard Model (SM) expectation. This tension can be relieved if the $W$ boson possesses a non-trivial right-handed gauge coupling at high energies. Such a right-handed gauge coupling induces by the SM gauge symmetric four-fermion interactions at TeV scales, where SM fermions...
The measurement of the sunrise azimuth on the sea horizon of Pescara is made in the season 1-march to 4-july (and more) by using a fixed reference point in the foreground, and the coordinates y to the horizon level and x towards left (+) or right (-). The parabola obtained in this way will be analyzed with modern tools now available in many spreadsheets softwares. The comparison with the...
The lecture will review the path that led to the observation of GRBs at High and Very High Energies.
I will review exact solutions to Einstein’s field equations coupled to dust and discuss their application to galaxies’ dynamic.
