22–26 Sept 2025
Moho
Europe/Paris timezone

Study of the isospin dependence of the temperature of different sources in the 78Kr+40 and 86Kr+48Ca reactions

Not scheduled
1m
Moho

Moho

16 bis Quai Hamelin 14000 CAEN
Poster Nuclear Structure, Spectroscopy and Dynamics Poster session

Speaker

Brunilde Gnoffo (Università degli Studi di Catania)

Description

Brunilde Gnoffo a,b, Sara Pirroneb , Giuseppe Politi a,b, Enrico De Filippob , Giuseppe Cardellab , Elena Geraci a,b, Concettina Maiolinoc , Nunzia Simona Martoranab , Emanuele Vincenzo Paganoc , Massimo Papab, Fabio Risitano d,b, Francesca Rizzoa,c,e, Paolo Russottoc , Marina Trimarchid,b, Cristina Zagamia,c,e
A Dipartimento di Fisica e Astronomia ”Ettore Majorana”, Universita degliStudidiCatania, via Santa Sofia 64, Catania, 95123, Italy,
b INFN Sezione di Catania, via Santa Sofia 64, Catania, 95123, Italy,
c INFN Laboratori Nazionali del Sud, via Santa Sofia 62, Catania, 95123, Italy,
d Dipartimento di Scienze Matematiche e Informatiche Scienze Fisiche e Scienze della Terra Universit degli Studi di Messina, Viale Ferdinando Stagno d’Alcontres, 31, Messina, 98166, Italy,
e CSFNSM-Centro Siciliano di Fisica Nucleare e Struttura della Materia, via Santa Sofia 64, Catania, 95123, Italy,

The influence of isospin on thermometric properties is examined in the reactions 78Kr + 40Ca and 86Kr + 48Ca at 10 AMeV. These reactions were realized as part of the ISODEC experiment at INFN-LNS (Laboratori Nazionali del Sud) in Catania, utilizing the 4π CHIMERA multidetector. The analysis of the collected data indicates a correlation between temperature and the N/Z ratio. Two thermometric approaches were employed to determine the temperature of different sources: the slope thermometer using alpha particles as a probe and the double isotope yield ratio method. The findings reveal that depending on the source, isospin affects the temperature differently. For example, for the compound nucleus source, the neutron-rich system exhibits higher temperatures compared to the neutron-poor one and this trend is further validated through comparisons with the GEMINI++ statistical model.

Authors

Brunilde Gnoffo (Università degli Studi di Catania) Sara Pirrone (INFN Sezione di Catania) Giuseppe POLITI (Dipartimento di Fisica e Astronomia - Università di Catania - ITALY)

Presentation materials

There are no materials yet.