activity
20052025
most citedDyonic Kerr-Newman black holes, complex scalar field and Cosmic Censorship

104 citations · 247 across the 12 of their papers we have counts for

collaborators

12 papers

gr-qc2025★ 2 cited

Analysis of Pantheon+ supernova data suggests evidence of sign-changing pressure of the cosmological fluid

A. Kazım Çamlıbel, M. Akif Feyizoğlu, İbrahim Semiz

In this work, we revisit/reinterpret/extend the model-independent analysis method (which we now call spread - luminosity distance fitting, spread-LDF) from our previous work. We ap…

gr-qc2022★ 10 cited

Weak field and slow motion limits in energy-momentum powered gravity

Ozgur Akarsu, A. Kazim Camlibel, Nihan Katirci +2

We explore the weak field and slow motion limits, Newtonian and Post-Newtonian limits, of the energy-momentum powered gravity (EMPG), viz., the energy-momentum squared gravity (EMS…

gr-qc2020★ 7 cited

The general static spherical perfect fluid solution with EoS parameter w=-1/5

İbrahim Semiz

The general analytical solution for the static spherically symmetric metric supported by a perfect fluid with isothermal (proportional) equation-of-state is not known at…

astro-ph.CO2020★ 36 cited

Pantheon update on a model-independent analysis of cosmological supernova data

A. K. Çamlıbel, İ. Semiz, M. A. Feyizoğlu

We present an update of our previous work, necessitated by availability of a significantly improved dataset. The work is a model-independent analysis of the cosmological supernova…

gr-qc2015★ 21 cited

Hawking radiation as the cosmic censor

Koray Düztaş, İbrahim Semiz

Hawking radiation acts as a cosmic censor since it carries away the angular momentum of the black hole, proportionally more than its mass. In this work we first show that an extrem…

gr-qc2015★ 2 cited

The decoupling problem of the Proca equation; and treatment of Dirac, Maxwell and Proca fields on the resulting pp-wave spacetimes

Koray Düztaş, İbrahim Semiz

In this work we take a formal approach to the problem of decoupling Proca equations in curved space-times. We use Newman-Penrose (NP) two-spinor formalism to represent the Proca ve…