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20032019
most citedNonlinear electrodynamics and the surface redshift of pulsars

58 citations · 158 across the 6 of their papers we have counts for

collaborators

6 papers

gr-qc2019★ 1 cited

How to distinguish an actual astrophysical magnetized black hole mimicker from a true (theoretical) black hole

A. Mitra, C. Corda, H. J. Mosquera Cuesta

We remind that the ring down features observed in the LIGO GWs resulted from trembling of photon spheres (Rp=3M) of newly formed compact objects and not from the trembling of their…

gr-qc2009★ 19 cited

A spherically symmetric and stationary universe from a weak modification of general relativity

Christian Corda, Herman J. Mosquera Cuesta

It is shown that a weak modification of general relativity, in the linearized approach, renders a spherically symmetric and stationary model of the universe. This is due to the pre…

astro-ph2008★ 25 cited

Neutrino mass spectrum from gravitational waves generated by double neutrino spin-flip in supernovae

Herman J. Mosquera Cuesta, Gaetano Lambiase

The supernova (SN) neutronization phase produces mainly electron () neutrinos, the oscillations of which must take place within a few mean-free-paths of their resonance surfac…

astro-ph2006★ 16 cited

Nonlinear electrodynamics and the Pioneer 10/11 spacecraft anomaly

Jean Paul Mbelek, Herman J. Mosquera Cuesta, M. Novello +1

The occurrence of the phenomenon known as photon acceleration is a natural prediction of nonlinear electrodynamics (NLED). This would appear as an anomalous frequency shift in any…

astro-ph2005★ 39 cited

Bardeen-Petterson effect and the disk structure of the Seyfert galaxy NGC 1068

Anderson Caproni, Zulema Abraham, Herman J. Mosquera Cuesta

VLBA high spatial resolution observations of the disk structure of the active galactic nucleus NGC 1068 has recently revealed that the kinematics and geometry of this AGN is well c…

astro-ph2003★ 58 cited

Nonlinear electrodynamics and the surface redshift of pulsars

Herman J. Mosquera Cuesta, Jose M. Salim

Currently is argued that the best method of determining the neutron star (NS) fundamental properties is by measuring the {\it gravitational redshift} () of spectral lines produc…