activity
20102026
most citedCosmological models with linearly varying deceleration parameter

198 citations · 1.8k across the 47 of their papers we have counts for

collaborators

49 papers

gr-qc2026

Gravitating sources with zero energy density in cosmology

Özgür Akarsu, Cihad Kıbrıs, Burcu Öztürk +1

A cosmological source can have identically zero comoving energy density and still gravitate through its pressure. This differs from an energy density passing through zero at an iso…

gr-qc2026

Reconstructing sign-switching dark energy histories: Scalar-field regularity, conditional potential comparison, and representative dynamics

Shahnawaz A. Adil, Özgür Akarsu, Mariam Bouhmadi-López +3

Phenomenologically similar sign-switching dark-energy histories need not have comparable scalar-field realizations. We reconstruct minimally coupled scalars with fixed kinetic sign…

gr-qc2026

Action-selected currents and a singular conservation closure in two-fluid energy--momentum-squared cosmology

Özgür Akarsu, Bilal Bulduk, Nihan Katırcı

In multi-fluid, matter-type gravity, the Bianchi identity constrains the divergence of the total effective stress tensor but does not, by itself, determine the currents assigned to…

gr-qc2026

Defocusing dark energy: Raychaudhuri diagnostics beyond and the phantom divide

Özgür Akarsu, Antonio De Felice, N. Merve Uzun

In general relativity, cosmic acceleration is timelike defocusing of the comoving congruence and requires a negative total active gravitational mass density, $\mathcal{M}_{\rm tot}…

astro-ph.CO2026

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families

Shahnawaz A. Adil, Miguel A. Zapata, Özgür Akarsu +1

We present a unified \emph{background-level} framework that maps a prescribed late-time dark-energy density history onto an effective scalar-field description in a…

astro-ph.CO2026

Probing dynamical dark energy with late-time data: Evidence, tensions, and the limits of the CDM framework

Tengpeng Xu, Suresh Kumar, Yun Chen +2

We test the dynamical dark-energy CDM (CPL) framework against CDM using CMB anisotropies and lensing together with DESI DR2, SDSS-IV, transverse/angular BAO (BAOtr), and…

gr-qc2025

k-inflation: Non-separable case meets ACT measurements

Tahere Fallahi Serish, Seyed Ali Hosseini Mansoori, Fereshteh Felegary +2

We investigate a non-separable subset of -essence in which the kinetic and potential sectors interact through an coupling, implemented via a potential-dependent prefac…

astro-ph.CO2025★ 12 cited

Linear matter density perturbations in the CDM model: Examining growth dynamics and addressing the tension

Özgür Akarsu, Arman Çam, Evangelos A. Paraskevas +1

We investigate linear matter density perturbations in the CDM, in which the is replaced by late-time () mirror AdS-dS transition, resulting in distinct growt…

astro-ph.CO2025★ 23 cited

Mapping the CDM scenario to modified gravity: Effects on structure growth rate

Mateus S. Souza, Ana M. Barcelos, Rafael C. Nunes +2

The concept of a rapidly sign-switching cosmological constant, interpreted as a mirror AdS-dS transition in the late universe and known as the CDM, has significantly imp…

gr-qc2024★ 17 cited

Unexplored regions in teleparallel gravity: Sign-changing dark energy density

Ozgur Akarsu, Bilal Bulduk, Antonio De Felice +2

While gravity has shown considerable potential in addressing cosmological tensions, we explore previously overlooked solution spaces that hold further promise. We examine th…

astro-ph.CO2024★ 23 cited

Exploring new physics in the late Universe's expansion through non-parametric inference

Miguel A. Sabogal, Özgür Akarsu, Alexander Bonilla +2

In this study, we investigate deviations from the Planck-CDM model in the late universe () using the Gaussian Processes method, with minimal assumptions. Our goa…

astro-ph.CO2024★ 28 cited

CDM cosmology: Alleviating major cosmological tensions by predicting standard neutrino properties

Anita Yadav, Suresh Kumar, Cihad Kibris +1

We investigate a two-parameter extension of the CDM model by allowing variations in the effective number of neutrino species and their total mass $\sum m_ν…

astro-ph.CO2024★ 38 cited

Cosmological constraints on CDM scenario in a type II minimally modified gravity

Özgür Akarsu, Antonio De Felice, Eleonora Di Valentino +5

The idea of a rapid sign-switching cosmological constant (mirror AdS-dS transition) in the late universe at , known as the CDM model, has significantly improve…

astro-ph.CO2024★ 10 cited

CDM cosmology from a type-II minimally modified gravity

Özgür Akarsu, Antonio De Felice, Eleonora Di Valentino +5

We integrate CDM, a promising scenario for alleviating cosmological tensions, into VCDM, a type-II minimally modified gravity. This promotes the scenario to a fully pred…

astro-ph.CO2024★ 31 cited

Transition dynamics in the CDM model: Implications for bound cosmic structures

Evangelos A. Paraskevas, Arman Cam, Leandros Perivolaropoulos +1

We explore the predictions of CDM, a novel framework suggesting a rapid anti-de Sitter (AdS) to de Sitter (dS) vacua transition in the late Universe, on bound cosmic str…

astro-ph.CO2024★ 51 cited

CDM Tensions: Localising Missing Physics through Consistency Checks

Özgür Akarsu, Eoin Ó Colgáin, Anjan A. Sen +1

CDM tensions are by definition model dependent; one sees anomalies through the prism of CDM. Thus, progress towards tension resolution necessitates checking the consistency o…

astro-ph.CO2023★ 10 cited

Quadratic energy-momentum squared gravity: constraints from big bang nucleosynthesis

Ozgur Akarsu, Mariam Bouhmadi-López, Nihan Katirci +1

In this work, we extend the standard cosmological model within the quadratic energy-momentum squared gravity (qEMSG) framework, introducing a nonminimal interaction between the usu…

gr-qc2023

Equivalence of matter-type modified gravity theories to general relativity with nonminimal matter interaction

Özgür Akarsu, Mariam Bouhmadi-López, Nihan Katırcı +3

In this study, we first establish that gravity models incorporating matter-related terms, such as , , and , into the usu…

astro-ph.CO2023★ 75 cited

Omnipotent dark energy: A phenomenological answer to the Hubble tension

Shahnawaz A. Adil, Ozgur Akarsu, Eleonora Di Valentino +4

This paper introduces the class of omnipotent dark energy (DE) models characterized by nonmonotonic energy densities that are capable of attaining negative values with correspondin…

astro-ph.CO2023★ 76 cited

Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Luis A. Escamilla, Ozgur Akarsu, Eleonora Di Valentino +1

The cosmological dark sector remains an enigma, offering numerous possibilities for exploration. One particularly intriguing option is the (non-minimal) interaction scenario betwee…

gr-qc2023★ 7 cited

Relativistic binary systems in scale-independent energy-momentum squared gravity

Ozgur Akarsu, Elham Nazari, Mahmood Roshan

In this paper, we study the gravitational-wave (GW) radiation and radiative behavior of relativistic binary systems in the scale-independent energy-momentum squared gravity (EMSG).…

astro-ph.CO2022★ 99 cited

Relaxing cosmological tensions with a sign switching cosmological constant: Improved results with Planck, BAO, and Pantheon data

Ozgur Akarsu, Suresh Kumar, Emre Ozulker +2

We present a further observational analysis of the CDM model proposed in Akarsu et al. [Phys. Rev. D 104, 123512 (2021)]. This model is based on the recent conjecture su…

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…

astro-ph.CO2022★ 31 cited

Inevitable manifestation of wiggles in the expansion of the late Universe

Ozgur Akarsu, Eoin O. Colgain, Emre Ozulker +2

Using the fact that the comoving angular diameter distance to the last scattering surface is strictly constrained almost model independently, we show that, for any model agreeing w…