The cascading 3.21 and 4.44 MeV electric quadrupole transitions have been observed from the Hoyle state at 7.65 MeV excitation energy in 12 C , excited by the 12 C ( p , p ′ ) reaction at 10.7 MeV proton energy. From the proton- γ − γ triple coincidence data, a value of Γ rad / Γ = 6.2 ( 6 ) x 10 − 4 was obtained for the radiative branching ratio. Using our results, together with Γ E 0 π / Γ from Eriksen et al. [Phys. Rev. C 102, 024320 (2020)] and the currently adopted Γ π ( E 0 ) values, the radiative width of the Hoyle state is determined as Γ rad = 5.1 ( 6 ) x 10 − 3 eV . This value is about 34% higher than the currently adopted value and will impact models of stellar evolution and nucleosynthesis.The project was supported by the Austra...
AbstractThe fragmentation of quasi-projectiles from the nuclear reaction 40Ca + 12C at 25 MeV/nucleo...
7 pags., 3 figs. -- International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos - IX, 25-...
By using the CHIMERA detector, we have measured the gamma-ray and alpha decay width of excited C-12 ...
This thesis focuses on a new determination of the radiative width, Γrad of the Hoyle state from the...
The triple-alpha process leading to the formation of stable carbon in the Universe is one of the mos...
International audience; The Hoyle state in 12C(Ex = 7.654MeV) is characterized by a pronounced 3α cl...
The αdecay path of the Hoyle state in 12C (Ex = 7:654MeV) represents one ofthe most challenging ques...
Using an array of high-purity Compton-suppressed germanium detectors, we performed an independent me...
The structure of the Hoyle state, a near-threshold 0+ state of extreme astrophysical significance in...
Precise estimation of the rare direct 3α decay of the Hoyle state of 12C has been made to unveil its...
The second 2+ state of the C12 nucleus is of great importance to nuclear astrophysics reaction rate ...
Excited states in certain atomic nuclei possess an unusual structure, where the dominant degrees of ...
We investigate an implication of the most recent observation of a second Jπ=2+ state in 12C, which w...
A low-lying Jπ = 2+ state in 12C was predicted over fifty years ago to exist as an excitation of the...
12C is synthesised in stars by fusion of three α particles. This process occurs through a resonance ...
AbstractThe fragmentation of quasi-projectiles from the nuclear reaction 40Ca + 12C at 25 MeV/nucleo...
7 pags., 3 figs. -- International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos - IX, 25-...
By using the CHIMERA detector, we have measured the gamma-ray and alpha decay width of excited C-12 ...
This thesis focuses on a new determination of the radiative width, Γrad of the Hoyle state from the...
The triple-alpha process leading to the formation of stable carbon in the Universe is one of the mos...
International audience; The Hoyle state in 12C(Ex = 7.654MeV) is characterized by a pronounced 3α cl...
The αdecay path of the Hoyle state in 12C (Ex = 7:654MeV) represents one ofthe most challenging ques...
Using an array of high-purity Compton-suppressed germanium detectors, we performed an independent me...
The structure of the Hoyle state, a near-threshold 0+ state of extreme astrophysical significance in...
Precise estimation of the rare direct 3α decay of the Hoyle state of 12C has been made to unveil its...
The second 2+ state of the C12 nucleus is of great importance to nuclear astrophysics reaction rate ...
Excited states in certain atomic nuclei possess an unusual structure, where the dominant degrees of ...
We investigate an implication of the most recent observation of a second Jπ=2+ state in 12C, which w...
A low-lying Jπ = 2+ state in 12C was predicted over fifty years ago to exist as an excitation of the...
12C is synthesised in stars by fusion of three α particles. This process occurs through a resonance ...
AbstractThe fragmentation of quasi-projectiles from the nuclear reaction 40Ca + 12C at 25 MeV/nucleo...
7 pags., 3 figs. -- International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos - IX, 25-...
By using the CHIMERA detector, we have measured the gamma-ray and alpha decay width of excited C-12 ...