Peripheral elastic and inelastic scattering of                          17,18                         O on light targets at 12 MeV/nucleon

F. Carstoiu; T. Al-Abdullah; C. A. Gagliardi; L. Trache

doi:10.1063/1.4909558

Peripheral elastic and inelastic scattering of ^17,18 O on light targets at 12 MeV/nucleon

F. Carstoiu, T. Al-Abdullah, C. A. Gagliardi, L. Trache

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

Abstract

The elastic and inelastic scattering of ^17,18 O with light targets has been undertaken at 12 MeV/nucleon in order to determine the optical potentials needed for the transfer reaction ¹³ C( ¹⁷ O, ¹⁸ O) ¹² C. Optical potentials in both incoming and outgoing channels have been determined in a single experiment. This transfer reaction was used to infer the direct capture rate to the ¹⁷ F(p,γ) ¹⁸ Ne which is essential to estimate the production of ¹⁸ F at stellar energies in ONe novae. We demonstrate the stability of the ANC method and OMP results using good quality elastic and inelastic scattering data with stable beams. The peripherality of our reaction is inferred from a semiclassical decomposition of the total scattering amplitude into barrier and internal barrier components. Comparison between elastic scattering of ¹⁷ O, ¹⁸ O and ¹⁶ O projectiles is made.

Original language	English
Title of host publication	Exotic Nuclei and Nuclear/Particle Astrophysics (V). From Nuclei to Stars - Carpathian Summer School of Physics 2014, CSSP 2014
Editors	Daniela Chesneanu, Livius Trache, Calin Alexandru Ur
Publisher	American Institute of Physics Inc.
Pages	39-51
Number of pages	13
ISBN (Electronic)	9780735412842
DOIs	https://doi.org/10.1063/1.4909558
State	Published - 2015
Externally published	Yes

Publication series

Name	AIP Conference Proceedings
Volume	1645
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Bibliographical note

Publisher Copyright:
© 2015 AIP Publishing LLC.

Keywords

WKB
Woods-Saxon potential
folding potentials

ASJC Scopus subject areas

General Physics and Astronomy

Access to Document

10.1063/1.4909558

Cite this

Carstoiu, F., Al-Abdullah, T., Gagliardi, C. A., & Trache, L. (2015). Peripheral elastic and inelastic scattering of ^17,18 O on light targets at 12 MeV/nucleon In D. Chesneanu, L. Trache, & C. A. Ur (Eds.), Exotic Nuclei and Nuclear/Particle Astrophysics (V). From Nuclei to Stars - Carpathian Summer School of Physics 2014, CSSP 2014 (pp. 39-51). (AIP Conference Proceedings; Vol. 1645). American Institute of Physics Inc.. https://doi.org/10.1063/1.4909558

Carstoiu, F. ; Al-Abdullah, T. ; Gagliardi, C. A. et al. / Peripheral elastic and inelastic scattering of ^17,18 O on light targets at 12 MeV/nucleon Exotic Nuclei and Nuclear/Particle Astrophysics (V). From Nuclei to Stars - Carpathian Summer School of Physics 2014, CSSP 2014. editor / Daniela Chesneanu ; Livius Trache ; Calin Alexandru Ur. American Institute of Physics Inc., 2015. pp. 39-51 (AIP Conference Proceedings).

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title = " Peripheral elastic and inelastic scattering of 17,18 O on light targets at 12 MeV/nucleon ",

abstract = " The elastic and inelastic scattering of 17,18 O with light targets has been undertaken at 12 MeV/nucleon in order to determine the optical potentials needed for the transfer reaction 13 C( 17 O, 18 O) 12 C. Optical potentials in both incoming and outgoing channels have been determined in a single experiment. This transfer reaction was used to infer the direct capture rate to the 17 F(p,γ) 18 Ne which is essential to estimate the production of 18 F at stellar energies in ONe novae. We demonstrate the stability of the ANC method and OMP results using good quality elastic and inelastic scattering data with stable beams. The peripherality of our reaction is inferred from a semiclassical decomposition of the total scattering amplitude into barrier and internal barrier components. Comparison between elastic scattering of 17 O, 18 O and 16 O projectiles is made.",

keywords = "WKB, Woods-Saxon potential, folding potentials",

author = "F. Carstoiu and T. Al-Abdullah and Gagliardi, \{C. A.\} and L. Trache",

note = "Publisher Copyright: {\textcopyright} 2015 AIP Publishing LLC.",

year = "2015",

doi = "10.1063/1.4909558",

language = "English",

series = "AIP Conference Proceedings",

publisher = "American Institute of Physics Inc.",

pages = "39--51",

editor = "Daniela Chesneanu and Livius Trache and Ur, \{Calin Alexandru\}",

booktitle = "Exotic Nuclei and Nuclear/Particle Astrophysics (V). From Nuclei to Stars - Carpathian Summer School of Physics 2014, CSSP 2014",

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Carstoiu, F, Al-Abdullah, T, Gagliardi, CA & Trache, L 2015, Peripheral elastic and inelastic scattering of ^17,18 O on light targets at 12 MeV/nucleon in D Chesneanu, L Trache & CA Ur (eds), Exotic Nuclei and Nuclear/Particle Astrophysics (V). From Nuclei to Stars - Carpathian Summer School of Physics 2014, CSSP 2014. AIP Conference Proceedings, vol. 1645, American Institute of Physics Inc., pp. 39-51. https://doi.org/10.1063/1.4909558

Peripheral elastic and inelastic scattering of ^17,18 O on light targets at 12 MeV/nucleon . / Carstoiu, F.; Al-Abdullah, T.; Gagliardi, C. A. et al.
Exotic Nuclei and Nuclear/Particle Astrophysics (V). From Nuclei to Stars - Carpathian Summer School of Physics 2014, CSSP 2014. ed. / Daniela Chesneanu; Livius Trache; Calin Alexandru Ur. American Institute of Physics Inc., 2015. p. 39-51 (AIP Conference Proceedings; Vol. 1645).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

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T1 - Peripheral elastic and inelastic scattering of 17,18 O on light targets at 12 MeV/nucleon

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AU - Al-Abdullah, T.

AU - Gagliardi, C. A.

AU - Trache, L.

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N2 - The elastic and inelastic scattering of 17,18 O with light targets has been undertaken at 12 MeV/nucleon in order to determine the optical potentials needed for the transfer reaction 13 C( 17 O, 18 O) 12 C. Optical potentials in both incoming and outgoing channels have been determined in a single experiment. This transfer reaction was used to infer the direct capture rate to the 17 F(p,γ) 18 Ne which is essential to estimate the production of 18 F at stellar energies in ONe novae. We demonstrate the stability of the ANC method and OMP results using good quality elastic and inelastic scattering data with stable beams. The peripherality of our reaction is inferred from a semiclassical decomposition of the total scattering amplitude into barrier and internal barrier components. Comparison between elastic scattering of 17 O, 18 O and 16 O projectiles is made.

AB - The elastic and inelastic scattering of 17,18 O with light targets has been undertaken at 12 MeV/nucleon in order to determine the optical potentials needed for the transfer reaction 13 C( 17 O, 18 O) 12 C. Optical potentials in both incoming and outgoing channels have been determined in a single experiment. This transfer reaction was used to infer the direct capture rate to the 17 F(p,γ) 18 Ne which is essential to estimate the production of 18 F at stellar energies in ONe novae. We demonstrate the stability of the ANC method and OMP results using good quality elastic and inelastic scattering data with stable beams. The peripherality of our reaction is inferred from a semiclassical decomposition of the total scattering amplitude into barrier and internal barrier components. Comparison between elastic scattering of 17 O, 18 O and 16 O projectiles is made.

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KW - Woods-Saxon potential

KW - folding potentials

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BT - Exotic Nuclei and Nuclear/Particle Astrophysics (V). From Nuclei to Stars - Carpathian Summer School of Physics 2014, CSSP 2014

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PB - American Institute of Physics Inc.

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Carstoiu F, Al-Abdullah T, Gagliardi CA, Trache L. Peripheral elastic and inelastic scattering of ^17,18 O on light targets at 12 MeV/nucleon In Chesneanu D, Trache L, Ur CA, editors, Exotic Nuclei and Nuclear/Particle Astrophysics (V). From Nuclei to Stars - Carpathian Summer School of Physics 2014, CSSP 2014. American Institute of Physics Inc. 2015. p. 39-51. (AIP Conference Proceedings). doi: 10.1063/1.4909558

Peripheral elastic and inelastic scattering of 17,18 O on light targets at 12 MeV/nucleon