Author

Trippella, Oscar

INSPIRE profile1423651 ORCID0000-0002-4757-0487

2 papers

Collaboratorsmost frequent first

	Paper	Category
Jan 24, 2020#142001.08316	Constraining the $^{22}$ Ne( $α$ , $γ$ ) $^{26}$ Mg and $^{22}$ Ne( $α$ ,n) $^{25}$ Mg reaction rates using sub-Coulomb $α$ -transfer reactions H. Jayatissa🇺🇸 · G.V. Rogachev🇺🇸 · V.Z. Goldberg🇺🇸 · E. Koshchiy🇺🇸 · G. Christian🇨🇦 · J. Hooker🇺🇸 · S. Ota🇯🇵 · B.T. Roeder🇺🇸 · A. Saastamoinen🇺🇸 · O. Trippella · S. Upadhyayula🇺🇸 · E. Uberseder🇺🇸	↳ nucl-ex	PLB	28
Feb 7, 2017#151702.01589	Concurrent application of ANC and THM to assess the $^{13} C (α, n)^{16} O$ absolute cross section at astrophysical energies and possible consequences for neutron production in low-mass AGB stars Oscar Trippella · Marco La Cognata	↳ astro-ph.SR	ApJ	34

Constraining the $^{22}$ Ne( $α$ , $γ$ ) $^{26}$ Mg and $^{22}$ Ne( $α$ ,n) $^{25}$ Mg reaction rates using sub-Coulomb $α$ -transfer reactions
H. Jayatissa🇺🇸 · G.V. Rogachev🇺🇸 · V.Z. Goldberg🇺🇸 · E. Koshchiy🇺🇸 · G. Christian🇨🇦 · J. Hooker🇺🇸 · S. Ota🇯🇵 · B.T. Roeder🇺🇸 · A. Saastamoinen🇺🇸 · O. Trippella · S. Upadhyayula🇺🇸 · E. Uberseder🇺🇸
Jan 24, 20202001.08316↳ nucl-exPLB28 citations
Concurrent application of ANC and THM to assess the $^{13} C (α, n)^{16} O$ absolute cross section at astrophysical energies and possible consequences for neutron production in low-mass AGB stars
Oscar Trippella · Marco La Cognata
Feb 7, 20171702.01589↳ astro-ph.SRApJ34 citations

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Trippella, Oscar

Constraining the 22Ne(α,γ)26Mg and 22Ne(α,n)25Mg reaction rates using sub-Coulomb α-transfer reactions

Concurrent application of ANC and THM to assess the 13C(α,n)16O absolute cross section at astrophysical energies and possible consequences for neutron production in low-mass AGB stars

Constraining the $^{22}$ Ne( $α$ , $γ$ ) $^{26}$ Mg and $^{22}$ Ne( $α$ ,n) $^{25}$ Mg reaction rates using sub-Coulomb $α$ -transfer reactions

Concurrent application of ANC and THM to assess the $^{13} C (α, n)^{16} O$ absolute cross section at astrophysical energies and possible consequences for neutron production in low-mass AGB stars