The reactions C-13(alpha,n)O-16 and Ne-22(alpha,n)Mg-25 are the primary sources of neutrons for the astrophysical s-process. The feasibility of cross section measurements within the respective Gamow windows is discussed in quantitative terms for a 4 pi neutron counter, based on He-3 tubes and a neutron moderator, placed in an underground lab
The 13C(α,n)16O reaction is the prevalent neutron source for the main s-process. The direct measurem...
The drive of low-energy nuclear astrophysics laboratories is to study the reactions of importance to...
The 13C(α,n)16O reaction is the prevalent neutron source for the main s-process. The direct measurem...
The reactions 13C(alpha, n)16O and 22Ne(alpha, n)25Mg are the primary sources of neutrons for the as...
The 13 C(α, n)16 O reaction determines the dominant neutron source of the sprocess in thermally puls...
The 13C(α, n)16O reaction determines the dominant neutron source of the sprocess in thermally pulsin...
The 13 C(α,n)16 O reaction is the prevalent neutron source for the main s-process. The direct measur...
INPC 2013 – International Nuclear Physics ConferenceWe present some open questions in nucleosynthesi...
One of the main neutron sources for the astrophysical s process is the reaction 13C(α,n)16O, taking ...
We present some open questions in nucleosynthesis focused on the measurement of relevant neutron cap...
The astrophysical p process unites all processes that have been introduced to explain the abundance ...
One of the main neutron sources for the astrophysical s process is the reaction C13(α,n)O16, taking ...
The 13C(α,n)16O reaction is the prevalent neutron source for the main s-process. The direct measurem...
The drive of low-energy nuclear astrophysics laboratories is to study the reactions of importance to...
The 13C(α,n)16O reaction is the prevalent neutron source for the main s-process. The direct measurem...
The reactions 13C(alpha, n)16O and 22Ne(alpha, n)25Mg are the primary sources of neutrons for the as...
The 13 C(α, n)16 O reaction determines the dominant neutron source of the sprocess in thermally puls...
The 13C(α, n)16O reaction determines the dominant neutron source of the sprocess in thermally pulsin...
The 13 C(α,n)16 O reaction is the prevalent neutron source for the main s-process. The direct measur...
INPC 2013 – International Nuclear Physics ConferenceWe present some open questions in nucleosynthesi...
One of the main neutron sources for the astrophysical s process is the reaction 13C(α,n)16O, taking ...
We present some open questions in nucleosynthesis focused on the measurement of relevant neutron cap...
The astrophysical p process unites all processes that have been introduced to explain the abundance ...
One of the main neutron sources for the astrophysical s process is the reaction C13(α,n)O16, taking ...
The 13C(α,n)16O reaction is the prevalent neutron source for the main s-process. The direct measurem...
The drive of low-energy nuclear astrophysics laboratories is to study the reactions of importance to...
The 13C(α,n)16O reaction is the prevalent neutron source for the main s-process. The direct measurem...
DOI
Add to ORKG