M. P. Tak'acs

activity

20152020

most citedDirect measurement of low-energy

^{22}

Ne(p,

γ

)

^{23}

Na resonances

55 citations · 269 across the 11 of their papers we have counts for

collaborators

Showing 2017Show all

3 papers · 1 filter

nucl-ex2017★ 34 cited

Astrophysical S-factor of the $^{14} N(p, γ)^{15} O$ reaction at 0.4 -- 1.3\,MeV

L. Wagner, S. Akhmadaliev, M. Anders +18

The $^{14} N(p, γ)^{15} O$ reaction is the slowest reaction of the carbon-nitrogen cycle of hydrogen burning and thus determines its rate. The precise knowl…

astro-ph.SR2017★ 14 cited

Constraining the $^{7}$ Be( $p, γ$ ) $^{8}$ B $S$ -factor with the new precise $^{7}$ Be solar neutrino flux from Borexino

Marcell P. Takács, Daniel Bemmerer, Arnd R. Junghans +1

Among the solar fusion reactions, the rate of the $^{7}$ Be( $p, γ$ ) $^{8}$ B reaction is one of the most difficult to determine rates. In a number of previous experiments, its astrophysica…

astro-ph.SR2017

Origin of meteoritic stardust unveiled by a revised proton-capture rate of $^{17}$ O

M. Lugaro, A. I. Karakas, C. G. Bruno +34

Stardust grains recovered from meteorites provide high-precision snapshots of the isotopic composition of the stellar environment in which they formed. Attributing their origin to…

Astrophysical S-factor of the 14N(p,γ)15O reaction at 0.4 -- 1.3\,MeV

Constraining the 7Be(p,γ)8B S-factor with the new precise 7Be solar neutrino flux from Borexino

Origin of meteoritic stardust unveiled by a revised proton-capture rate of 17O

Astrophysical S-factor of the $^{14} N(p, γ)^{15} O$ reaction at 0.4 -- 1.3\,MeV

Constraining the $^{7}$ Be( $p, γ$ ) $^{8}$ B $S$ -factor with the new precise $^{7}$ Be solar neutrino flux from Borexino

Origin of meteoritic stardust unveiled by a revised proton-capture rate of $^{17}$ O