Using an array of high-purity Compton-suppressed germanium detectors, we performed an independent measurement of the β-decay branching ratio from 12B to the second-excited state, also known as the Hoyle state, in 12C. Our result is 0.64(11)%, which is a factor ∼2 smaller than the previously established literature value, but is in agreement with another recent measurement. This could indicate that the Hoyle state is more clustered than previously believed. The angular correlation of the Hoyle state γ cascade has also been measured for the first time. It is consistent with theoretical predictions.Fil: Munch, M.. University Aarhus; DinamarcaFil: Alcorta, M.. Westbrook Mall; Canadá. Argonne National Laboratory; Estados UnidosFil: Fynbo, H. O. U...
A low-lying Jπ = 2+ state in 12C was predicted over fifty years ago to exist as an excitation of the...
The second 2+ state of the C12 nucleus is of great importance to nuclear astrophysics reaction rate ...
The triple-alpha process leading to the formation of stable carbon in the Universe is one of the mos...
Using an array of high-purity Compton-suppressed germanium detectors, we performed an independent me...
The cascading 3.21 and 4.44 MeV electric quadrupole transitions have been observed from the Hoyle st...
Excited states in certain atomic nuclei possess an unusual structure, where the dominant degrees of ...
Precise estimation of the rare direct 3α decay of the Hoyle state of 12C has been made to unveil its...
The β-decay branching ratio of 12B to the Hoyle state in 12C was measured by detection of γ rays. 12...
We investigate an implication of the most recent observation of a second Jπ=2+ state in 12C, which w...
This thesis focuses on a new determination of the radiative width, Γrad of the Hoyle state from the...
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...
Background: The structure of the Hoyle state, a highly α-clustered state at 7.65 MeV in C12, has lon...
The structure of the Hoyle state, a near-threshold 0+ state of extreme astrophysical significance in...
By using the CHIMERA detector, we have measured the gamma-ray and alpha decay width of excited C-12 ...
A low-lying Jπ = 2+ state in 12C was predicted over fifty years ago to exist as an excitation of the...
The second 2+ state of the C12 nucleus is of great importance to nuclear astrophysics reaction rate ...
The triple-alpha process leading to the formation of stable carbon in the Universe is one of the mos...
Using an array of high-purity Compton-suppressed germanium detectors, we performed an independent me...
The cascading 3.21 and 4.44 MeV electric quadrupole transitions have been observed from the Hoyle st...
Excited states in certain atomic nuclei possess an unusual structure, where the dominant degrees of ...
Precise estimation of the rare direct 3α decay of the Hoyle state of 12C has been made to unveil its...
The β-decay branching ratio of 12B to the Hoyle state in 12C was measured by detection of γ rays. 12...
We investigate an implication of the most recent observation of a second Jπ=2+ state in 12C, which w...
This thesis focuses on a new determination of the radiative width, Γrad of the Hoyle state from the...
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...
Background: The structure of the Hoyle state, a highly α-clustered state at 7.65 MeV in C12, has lon...
The structure of the Hoyle state, a near-threshold 0+ state of extreme astrophysical significance in...
By using the CHIMERA detector, we have measured the gamma-ray and alpha decay width of excited C-12 ...
A low-lying Jπ = 2+ state in 12C was predicted over fifty years ago to exist as an excitation of the...
The second 2+ state of the C12 nucleus is of great importance to nuclear astrophysics reaction rate ...
The triple-alpha process leading to the formation of stable carbon in the Universe is one of the mos...