The structure of the Hoyle state and its 2+ partner state in 12C

We have measured the 12C(γ, 3α) reaction with an Optical Time Projection Chamber (O-TPC) detector operating with the CO2(80%) + N2(20%) gas mixture and gamma-ray beams from the HIγS facility of the TUNL at Duke. We measured complete angular distributions (between 9.1 – 10.7 MeV) from which we determ...

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Bibliographic Details
Main Author: Gai Moshe
Format: Article
Language:English
Published: EDP Sciences 2012-12-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20123815001
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spelling doaj-4088d6fef9a140cea5b326806489300e2021-08-02T09:35:14ZengEDP SciencesEPJ Web of Conferences2100-014X2012-12-01381500110.1051/epjconf/20123815001The structure of the Hoyle state and its 2+ partner state in 12CGai MosheWe have measured the 12C(γ, 3α) reaction with an Optical Time Projection Chamber (O-TPC) detector operating with the CO2(80%) + N2(20%) gas mixture and gamma-ray beams from the HIγS facility of the TUNL at Duke. We measured complete angular distributions (between 9.1 – 10.7 MeV) from which we determine the cross section yield curve and E1 – E2 relative phases leading to an unambiguous identification of the second 2+ state in 12C at 10.03(11) MeV. The observed spectrum of 12C below 12 MeV including the 22+ state observed in this work resembles the rotation-vibration spectrum predicted for a triangular shape oblate spinning top in which the Hoyle state is the first vibrational breathing mode of the triangular three alpha-particle system. We also observed a hint of the 23+ state which is predicted by the U(7) model as a member of the 1- bending mode band, but the existence of this 23+ is yet to be confirmed. The predicted rotation-vibration spectrum of a triangular shape oblate spinning top (with a D3h symmetry) allows us to compare the moment of inertia of the predicted Hoyle rotational band to the ground state rotational band and in this way extract the (large) rms radius of the Hoyle state of 3.22(8) fm. We compare the deduced rms radius with recent ab-initio theories and cluster models as well as the radius extracted from 12C(p, p′) data. http://dx.doi.org/10.1051/epjconf/20123815001
collection DOAJ
language English
format Article
sources DOAJ
author Gai Moshe
spellingShingle Gai Moshe
The structure of the Hoyle state and its 2+ partner state in 12C
EPJ Web of Conferences
author_facet Gai Moshe
author_sort Gai Moshe
title The structure of the Hoyle state and its 2+ partner state in 12C
title_short The structure of the Hoyle state and its 2+ partner state in 12C
title_full The structure of the Hoyle state and its 2+ partner state in 12C
title_fullStr The structure of the Hoyle state and its 2+ partner state in 12C
title_full_unstemmed The structure of the Hoyle state and its 2+ partner state in 12C
title_sort structure of the hoyle state and its 2+ partner state in 12c
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2012-12-01
description We have measured the 12C(γ, 3α) reaction with an Optical Time Projection Chamber (O-TPC) detector operating with the CO2(80%) + N2(20%) gas mixture and gamma-ray beams from the HIγS facility of the TUNL at Duke. We measured complete angular distributions (between 9.1 – 10.7 MeV) from which we determine the cross section yield curve and E1 – E2 relative phases leading to an unambiguous identification of the second 2+ state in 12C at 10.03(11) MeV. The observed spectrum of 12C below 12 MeV including the 22+ state observed in this work resembles the rotation-vibration spectrum predicted for a triangular shape oblate spinning top in which the Hoyle state is the first vibrational breathing mode of the triangular three alpha-particle system. We also observed a hint of the 23+ state which is predicted by the U(7) model as a member of the 1- bending mode band, but the existence of this 23+ is yet to be confirmed. The predicted rotation-vibration spectrum of a triangular shape oblate spinning top (with a D3h symmetry) allows us to compare the moment of inertia of the predicted Hoyle rotational band to the ground state rotational band and in this way extract the (large) rms radius of the Hoyle state of 3.22(8) fm. We compare the deduced rms radius with recent ab-initio theories and cluster models as well as the radius extracted from 12C(p, p′) data.
url http://dx.doi.org/10.1051/epjconf/20123815001
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