CINECA IRIS Institutional Research Information System
IRIS è l'Anagrafe della ricerca dell'Università degli Studi di Trento, e ha lo scopo di raccogliere, documentare, conservare e diffondere, anche ad accesso aperto, la produzione scientifica degli autori afferenti all'Università degli Studi di Trento.
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Contatto: iris@unitn.itPubblicazioni recenti
r-Process Nucleosynthesis in the Early Universe Through Fast Mergers of Compact Binaries in Triple Systems
Surface abundance observations of halo stars hint at the occurrence of r-process nucleosynthesis at low metallicity ([Fe/H] < -3), possibly within the first 108 yr after the formation of the first stars. Possible loci of early-Universe r-process nucleosynthesis are the ejecta of&...
Methods for the analysis of time series of multispectral remote sensing images and application to climate change variable estimations
In the last decades, the increasing number of new generation satellite images characterized by a better spectral, spatial and temporal resolution with respect to the past has provided unprecedented source of information for monitoring climate changes.To exploit this wealth of data, pow...
Gravitational-wave luminosity of binary neutron stars mergers
We study the gravitational-wave peak luminosity and radiated energy of quasicircular neutron star mergers using a large sample of numerical relativity simulations with different binary parameters and input physics. The peak luminosity for all the binaries can be described in terms of th...
Clinical self-tracking to improve knowing in practice: designing self-experiments for Type 2 Diabetes care
This thesis positions itself within the stream of research on self-tracking practices for the management of chronic illnesses. Self-care technologies, such as smartphones and many other mobile health devices, have led to the production of health data of patients outside institutional setting...
Light-curve models of black hole - neutron star mergers: Steps towards a multi-messenger parameter estimation
In the new era of gravitational wave (GW) and multi-messenger astrophysics, the detection of a GW signal from the coalescence of a black hole - neutron star (BHNS) binary remains a highly anticipated discovery. This system is expected to be within reach of the second gene...
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