Search for 22Na in novae supported by a novel method for measuring femtosecond nuclear lifetimes

Abstract Classical novae are thermonuclear explosions in stellar binary systems, and important sources of 26Al and 22Na. While γ rays from the decay of the former radioisotope have been observed throughout the Galaxy, 22Na remains untraceable. Its half-life (2.6 yr) would allow the observation of it...

Full description

Bibliographic Details
Main Authors: Chloé Fougères, François de Oliveira Santos, Jordi José, Caterina Michelagnoli, Emmanuel Clément, Yung Hee Kim, Antoine Lemasson, Valdir Guimarães, Diego Barrientos, Daniel Bemmerer, Giovanna Benzoni, Andrew J. Boston, Roman Böttger, Florent Boulay, Angela Bracco, Igor Čeliković, Bo Cederwall, Michał Ciemala, Clément Delafosse, César Domingo-Pardo, Jérémie Dudouet, Jürgen Eberth, Zsolt Fülöp, Vicente González, Andrea Gottardo, Johan Goupil, Herbert Hess, Andrea Jungclaus, Ayşe Kaşkaş, Amel Korichi, Silvia M. Lenzi, Silvia Leoni, Hongjie Li, Joa Ljungvall, Araceli Lopez-Martens, Roberto Menegazzo, Daniele Mengoni, Benedicte Million, Jaromír Mrázek, Daniel R. Napoli, Alahari Navin, Johan Nyberg, Zsolt Podolyák, Alberto Pullia, Begoña Quintana, Damien Ralet, Nadine Redon, Peter Reiter, Kseniia Rezynkina, Frédéric Saillant, Marie-Delphine Salsac, Angel M. Sánchez-Benítez, Enrique Sanchis, Menekşe Şenyiğit, Marco Siciliano, Nadezda A. Smirnova, Dorottya Sohler, Mihai Stanoiu, Christophe Theisen, Jose J. Valiente-Dobón, Predrag Ujić, Magdalena Zielińska
Format: Article
Language:English
Published: Nature Portfolio 2023-09-01
Series:Nature Communications
Online Access:https://doi.org/10.1038/s41467-023-40121-3