Neutron energy spectra following radiative pion absorption on 16O and 28Si nuclei

The energy spectra of neutrons between 2 and 28 MeV emitted following radiative pion capture in carbon, oxygen, and calcium fall off exponentially. An enhancement, however, is observed for neutron energies below 5 MeV in carbon and oxygen. Neutron yield peaks at n-y angles of 180', indicating a quasifree absorption mechanism in this process. ' NUCLEAa aEACTIONS "C(r-, ny~, "O~~-, nq), 4'Ca~~, ny),~= 0 MeV;" measured reaction rate, neutron energy spectrum, and n-y angular correlations"deduced giant resonance states and direct emission contributions .

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Effects of the Giant Resonance on the Energy Spectra of Neutrons Emitted Following Muon Capture inC12and
Plett
¹
,
Sobottka
²

1971
Phys. Rev. C
15
1
5
0
View full text Add to dashboard Cite

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Neutron energy spectra following radiative pion absorption on 16O and 28Si nuclei

Cited by 4 publications

References 10 publications

Excitation of isobaric analogue states in meson-induced nuclear reactions

Excitation of isobaric analogue states in meson-induced nuclear reactions

Neutrons from radiative pion capture in carbon, oxygen, and calcium

Effects of the Giant Resonance on the Energy Spectra of Neutrons Emitted Following Muon Capture inC12and
Plett
¹
,
Sobottka
²

1971
Phys. Rev. C
15
1
5
0
View full text Add to dashboard Cite

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Neutron energy spectra following radiative pion absorption on 16O and 28Si nuclei

Cited by 4 publications

References 10 publications

Excitation of isobaric analogue states in meson-induced nuclear reactions

Excitation of isobaric analogue states in meson-induced nuclear reactions

Neutrons from radiative pion capture in carbon, oxygen, and calcium

Effects of the Giant Resonance on the Energy Spectra of Neutrons Emitted Following Muon Capture inC12andPlett1, Sobottka2 1971Phys. Rev. C15150View full textAdd to dashboardCite

Contact Info

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Effects of the Giant Resonance on the Energy Spectra of Neutrons Emitted Following Muon Capture inC12and
Plett
¹
,
Sobottka
²

1971
Phys. Rev. C
15
1
5
0
View full text Add to dashboard Cite