activity
20052026
most citedThe Limits of Bound Structures in the Accelerating Universe

58 citations · 126 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

The ionised interstellar medium of DSFGs revealed by JWST/NIRSpec and ALMA: Super-solar metallicity, low ionisation parameters and, typical electron densities

Steven Gillman, Kei Ito, Francesco Valentino +25

We present a detailed study of near-infrared (2-4m) JWST/NIRSpec spectra of 48 high-redshift () galaxies detected with ALMA at . From a multi-wa…

math.PR2025

Characterisation of Markov property on planar maps

Pablo Araya, Luis Fredes, Avelio Sepúlveda

We revisit, in a self contained way, the Markov property on planar maps and decorated planar maps from three perspectives. First, we characterize the laws on these planar maps that…

astro-ph2007★ 38 cited

Hall drift of axisymmetric magnetic fields in solid neutron-star matter

Andreas Reisenegger, Rafael Benguria, Joaquin P. Prieto +2

Hall drift, i. e., transport of magnetic flux by the moving electrons giving rise to the electrical current, may be the dominant effect causing the evolution of the magnetic field…

astro-ph2006★ 18 cited

Redshift-space limits of bound structures

Rolando Dünner, Andreas Reisenegger, Andrés Meza +2

An exponentially expanding Universe, possibly governed by a cosmological constant, forces gravitationally bound structures to become more and more isolated, eventually becoming cau…

astro-ph2006★ 58 cited

The Limits of Bound Structures in the Accelerating Universe

Rolando Dünner, Pablo A. Araya, Andrés Meza +1

According to the latest evidence, the Universe is entering an era of exponential expansion, where gravitationally bound structures will get disconnected from each other, forming is…

astro-ph2005★ 12 cited

Magnetic fields in neutron stars: A theoretical perspective

Andreas Reisenegger, Joaquin Prieto, Rafael Benguria +2

We present our view of the main physical ingredients determining the evolution of neutron star magnetic fields. This includes the basic properties of neutron star matter, possible…