activity
20012026
most citedDN interaction from meson exchange

103 citations · 843 across the 36 of their papers we have counts for

collaborators

36 papers

hep-ph2026

Scattering and Femtoscopic Correlation Functions of the , and Systems

Mikel F. Barbat, Juan Nieves, Laura Tolos

We present predictions for scattering observables and femtoscopic correlation functions (CFs) of the , systems and its heavy-flavor counterpart…

hep-ph2024★ 17 cited

Masquerading hybrid stars with dark matter

Carline Biesdorf, Jürgen Schaffner-Bielich, Laura Tolos

We investigate the influence of dark matter on hybrid stars. Using a two-fluid approach, where normal and dark matter components interact only gravitationally, we explore how dark…

hep-ph2024★ 9 cited

Thermodynamic Consistent Description of Compact Stars of Two Interacting Fluids: The Case of Neutron Stars with Higgs Portal Dark Matter

Fazlollah Hajkarim, Jürgen Schaffner-Bielich, Laura Tolos

We consider a thermodynamically consistent approach for the computation of the masses, radii, and tidal deformabilities of compact stars consisting of two interacting fluids with s…

nucl-th2024★ 4 cited

On the determination of the meson width in the nuclear medium with the transparency ratio

Victor Montesinos, Natsumi Ikeno, Eulogio Oset +3

We have studied the feasibility of the experimental determination of the width of a meson in a nuclear medium by using the method of the nuclear transparency. The cross section…

astro-ph.HE2024★ 47 cited

Comprehensive study of compact stars with dark matter

Mikel F. Barbat, Jürgen Schaffner-Bielich, Laura Tolos

We present a comprehensive study of compact stars admixed with non-self annihilating self-interacting fermionic dark matter, delineating the dependence on the nuclear equation of s…

hep-ph2024★ 5 cited

Charge-conjugation asymmetry and molecular content: the in matter

Victor Montesinos, Miguel Albaladejo, Juan Nieves +1

We analyze the modifications that a dense nuclear medium induces in the and . In the vacuum, we consider them as isoscalar and…