Massive black hole factories: Supermassive and quasi-star formation in primordial halos

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A new paradigm to allow faster convergence rate is proposed for iterative regularization gradient-like descent approaches. The key idea consists of modifying the conventional

Osservando invece l’indice di dispersione R per le varie tipologie si nota che le differenze si fanno molto più marcate, passando da un minimo di 0,38 ad un massimo di 0,95: i

While a good agreement on the formation mechanisms of the stellar population has been reached, with SBHs forming at the end of the life of stars with masses ∼ > 20 M ⊙ or when

Simulation results show that the GE1/1 measurement station is suitable for running in the CMS high η background environment and will be crucial in controlling muon trigger rate and

The accuracy with which the amount of material in the ID is known contributes the largest source of uncertainty on the simulation-based estimate of the track reconstruction

— We present the result of an empirical model for elastic pp scattering at LHC which indicates that the asymptotic black disk limit R = σ elastic /σ total →.. 1/2 is not yet reached

Firstly, theoretical introduction explained as Agent-Based Modelling and Import processes, it is performed through research on the literature and Flexible Large-scale Agent