34 citations · 64 across the 5 of their papers we have counts for
5 papers
How Jupiters save or destroy inner Neptunes around evolved stars
María Paula Ronco, Matthias R. Schreiber, Cristian A. Giuppone +3
In about 6 Giga years our Sun will evolve into a red giant and finally end its life as a white dwarf. This stellar metamorphosis will occur to virtually all known host stars of exo…
Planetesimal fragmentation and giant planet formation II: dependencies with planetesimal relative velocities and compositions
I. L. San Sebastián, O. M. Guilera, M. G. Parisi
Most of planet formation models that incorporate planetesimal fragmentation consider a catastrophic impact energy threshold for basalts at a constant velocity of 3 km/s during all…
Effects of Hadron-Quark Phase Transitions in Hybrid Stars within the NJL Model
Ignacio Francisco Ranea-Sandoval, Milva Gabriela Orsaria, Germán Malfatti +4
We study local and non-local Polyakov Nambu-Jona-Lasinio models and analyze their respective phase transition diagram. We construct hybrid stars using the zero temperature limit of…
Hybrid magnetized stars within the Field Correlator Method
Mauro Mariani, Milva G. Orsaria, Ignacio F. Ranea-Sandoval +1
We present preliminary results of the study of intense magnetic fields effects on hybrid stars. For the description of the hadronic phase, we use the relativistic mean field approx…
Planetesimal fragmentation and giant planet formation: the role of planet migration
O. M. Guilera, D. Swoboda, Y. Alibert +3
In the standard model of core accretion, the cores of the giant planets form by the accretion of planetesimals. In this scenario, the evolution of the planetesimal population plays…