12C(20Ne, 16O)16O α-transfer reaction and astrophysical S-factors at 300keV

Author:

Mondal Ashok Kumar1,Basu C.1ORCID,Adhikari S.2,Bhattacharya C.34,Rana T. K.34,Kundu S.34,Manna S.34,Pandey R.3,Roy P.34,Sen A.34,Meena J. K.3,Saha A. K.3,Sahoo J. K.3,Basak Dipali1,Bar Tanmay1,Pai Haridas1,Bisoi A.5,Mitra A. K.1,Biswas Piyasi1

Affiliation:

1. Nuclear Physics Division, Saha Institute Of Nuclear Physics, HBNI, 1/AF Bidhan Nagar, Kolkata-700064, India

2. Techno India University, EM-4/1, Sector-V, Salt Lake, Kolkata-700091, India

3. Variable Energy Cyclotron Centre, Kolkata-700064, India

4. Homi Bhabha National Institute, Training school complex, Anushakti Nagar, Mumbai- 400094, India

5. Indian Institute of Engineering Science and Technology, Shibpur, Howrah-711103, India

Abstract

The [Formula: see text]C([Formula: see text]Ne, [Formula: see text]O)[Formula: see text]O reaction has been used for the first time to determine ANC of [Formula: see text]O levels. The [Formula: see text]C([Formula: see text]Ne, [Formula: see text]O)[Formula: see text]O [Formula: see text]-transfer angular distributions are measured at [Formula: see text][Formula: see text]MeV and used to determine the ANC of the ground, 6.05[Formula: see text]MeV ([Formula: see text]), 6.13[Formula: see text]MeV ([Formula: see text]), 6.92[Formula: see text]MeV ([Formula: see text]) and 7.12[Formula: see text]MeV ([Formula: see text]) states of [Formula: see text]O. The ANC values are [Formula: see text] [Formula: see text] [Formula: see text], [Formula: see text] [Formula: see text], [Formula: see text] [Formula: see text], [Formula: see text] [Formula: see text] and [Formula: see text] [Formula: see text]. Astrophysical S-factors at 300[Formula: see text]keV are extracted [Formula: see text]) keV b and [Formula: see text] keV b[Formula: see text] using these ANC values by R-matrix theory.

Publisher

World Scientific Pub Co Pte Lt

Subject

General Physics and Astronomy,Nuclear and High Energy Physics

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