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Search for $^{22}$Na in novae supported by a novel method for measuring femtosecond nuclear lifetimes
Classical novae are thermonuclear explosions in stellar binary systems, and important sources of $^{26}$Al and $^{22}$Na. While γ rays from the decay of the former radioisotope have been observed throughout the Galaxy, $^{22}$Na remains untraceable. Its half-life (2.6 yr) would allow the observation...
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