activity
20102022
most citedConstraints on Perturbative f(R) Gravity via Neutron Stars

223 citations · 321 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.HE2022★ 3 cited

Intra-pulse variability induced by plasmoid formation in pulsar magnetospheres

I. Ceyhun Andaç, Benoît Cerutti, Guillaume Dubus +1

Pulsars show irregularities in their pulsed radio emission that originate from propagation effects and the intrinsic activity of the source. In this work, we investigate the role p…

astro-ph.HE2021★ 1 cited

Evolution of proto-neutron stars to pulsars, magnetars and central compact objects

İrem Bakır, Kazım Yavuz Ekşi

Some young neutron stars, the magnetars, have ultra-strong magnetic fields, yet their inferred birth rate is comparable to the core-collapse supernova rate, challenging scenarios t…

astro-ph.HE2017★ 9 cited

On the morphology of outbursts of accreting millisecond X-ray pulsar Aquila X-1

Can Güngör, Kazım Yavuz Ekşi, Ersin Göğüş

We present the X-ray light curves of the last two outbursts --2014 & 2016-- of the well known accreting millisecond X-ray pulsar (AMXP) Aquila X-1 using the monitor of all sky X-ra…

gr-qc2016★ 9 cited

Relativistic stars in Starobinsky gravity with the matched asymptotic expansions method

Savaş Arapoğlu, Sercan Çıkıntoğlu, K. Yavuz Ekşi

We study the structure of relativistic stars in theory using the method of matched asymptotic expansion to handle the higher order derivatives in fie…

gr-qc2015★ 11 cited

Moment of inertia of neutron star crust in alternative and modified theories of gravity

Kalin Staykov, K. Yavuz Ekşi, Stoytcho S. Yazadjiev +2

The glitch activity of young pulsars arises from the exchange of angular momentum between the crust and the interior of the star. Recently, it was inferred that the moment of inert…

astro-ph.HE2014★ 14 cited

The Vela Pulsar With an Active Fallback Disk

Gökçe Özsükan, K. Yavuz Ekşi, Valeri Hambaryan +4

Fallback disks are expected to form around young neutron stars. The presence of these disks can be revealed by their blackbody spectrum in the infrared, optical and UV bands. We pr…