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Autor:
Liang, Johnson
In classical novae, the endpoint of nucleosynthesis occurs near A ~ 40. Currently, observations of classical novae predict an order of magnitude enhancement of endpoint elements, such as Ar, K, and Ca, relative to solar abundances; however, simulatio
Externí odkaz:
http://hdl.handle.net/11375/26019
Autor:
Liang, Johnson
Explosive events in our universe provide an environment where rare nucleosynthesis events can occur. Understanding the mechanisms and processes during these events is integral to understanding the relative abundances of the elements in our universe.
Externí odkaz:
http://hdl.handle.net/11375/20607
Autor:
Setoodehnia, Kiana, Marshall, Caleb, Longland, Richard, Kelley, John H., Liang, Johnson, Chaves, Federico Portillo
Background: Discrepancies exist between the observed abundances of argon and calcium in oxygen-neon nova ejecta and those predicted by nova models. An improved characterization of the $^{38}$K($p, \gamma$)$^{39}$Ca reaction rate over the nova tempera
Externí odkaz:
http://arxiv.org/abs/1811.00398
Autor:
Liang, Johnson
Explosive events in our universe provide an environment where rare nucleosynthesis events can occur. Understanding the mechanisms and processes during these events is integral to understanding the relative abundances of the elements in our universe.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1154::2f6239b9664d14a64c37991a0879f271
http://hdl.handle.net/11375/20607
http://hdl.handle.net/11375/20607