X. Viñas
University of Barcelona
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Publication
Featured researches published by X. Viñas.
Physical Review Letters | 2009
M. Centelles; X. Roca-Maza; X. Viñas; M. Warda
We describe a relation between the symmetry energy coefficients c(sym)(rho) of nuclear matter and a(sym)(A) of finite nuclei that accommodates other correlations of nuclear properties with the low-density behavior of c(sym)(rho). Here, we take advantage of this relation to explore the prospects for constraining c(sym)(rho) of systematic measurements of neutron skin sizes across the mass table, using as example present data from antiprotonic atoms. The found constraints from neutron skins are in harmony with the recent determinations from reactions and giant resonances.
Physical Review Letters | 2011
X. Roca-Maza; M. Centelles; X. Viñas; M. Warda
A precise determination of the neutron skin Δr(np) of a heavy nucleus sets a basic constraint on the nuclear symmetry energy (Δr(np) is the difference of the neutron and proton rms radii of the nucleus). The parity radius experiment (PREX) may achieve it by electroweak parity-violating electron scattering (PVES) on (208)Pb. We investigate PVES in nuclear mean field approach to allow the accurate extraction of Δr(np) of (208)Pb from the parity-violating asymmetry A(PV) probed in the experiment. We demonstrate a high linear correlation between A(PV) and Δr(np) in successful mean field forces as the best means to constrain the neutron skin of (208)Pb from PREX, without assumptions on the neutron density shape. Continuation of the experiment with higher precision in A(PV) is motivated since the present method can support it to constrain the density slope of the nuclear symmetry energy to new accuracy.
Physical Review C | 2009
M. Warda; X. Viñas; X. Roca-Maza; M. Centelles
We analyze the neutron skin thickness in finite nuclei with the droplet model and effective nuclear interactions. The ratio of the bulk symmetry energy
Physical Review C | 2011
X. Roca-Maza; X. Viñas; M. Centelles; P. Ring; P. Schuck
J
Nuclear Physics | 2004
M. Baldo; C. Maieron; P. Schuck; X. Viñas
to the so-called surface stiffness coefficient
Physical Review C | 2001
M. Del Estal; M. Centelles; X. Viñas; S. K. Patra
Q
Physical Review C | 2013
X. Roca-Maza; M. Brenna; G. Colò; M. Centelles; X. Viñas; B. K. Agrawal; Nils Paar; Dario Vretenar; J. Piekarewicz
has in the droplet model a prominent role in driving the size of neutron skins. We present a correlation between the density derivative of the nuclear symmetry energy at saturation and the
Physics Letters B | 2008
Marcello Baldo; P. Schuck; X. Viñas
J/Q
Physical Review C | 2001
S. K. Patra; M. Del Estal; M. Centelles; X. Viñas
ratio. We emphasize the role of the surface widths of the neutron and proton density profiles in the calculation of the neutron skin thickness when one uses realistic mean-field effective interactions. Next, taking as experimental baseline the neutron skin sizes measured in 26 antiprotonic atoms along the mass table, we explore constraints arising from neutron skins on the value of the
Physical Review C | 2010
M. Warda; X. Viñas; X. Roca-Maza; M. Centelles
J/Q