40 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- University of ZululandZA10 papers
- National Institute for Theoretical PhysicsZA4 papers
- Netaji Subhas University of TechnologyIN4 papers
- GLA UniversityIN3 papers
- University of KwaZulu-NatalZA3 papers
- North-West UniversityZA2 papers
- Stellenbosch UniversityZA2 papers
- Adekunle Ajasin UniversityNG1 paper
- Beijing Normal UniversityCN1 paper
- Chinese Academy of SciencesCN1 paper
- Galgotias UniversityIN1 paper
- G.L. Bajaj Institute of Technology and Management Greater NoidaIN1 paper
5 papers · 1 filter
Cross-correlation between the thermal Sunyaev-Zeldovich effect and the Integrated Sachs-Wolfe effect
Ayodeji Ibitoye, Wei-Ming Dai, Yin-Zhe Ma +5
We present a joint cosmological analysis of the power spectra measurement of the Planck Compton parameter and the integrated Sachs-Wolfe (ISW) maps. We detect the statistical corre…
CoLFI: Cosmological Likelihood-free Inference with Neural Density Estimators
Guo-Jian Wang, Cheng Cheng, Yin-Zhe Ma +3
In previous works, we proposed to estimate cosmological parameters with the artificial neural network (ANN) and the mixture density network (MDN). In this work, we propose an impro…
Reconstruction of an Observationally Constrained gravity model
Anirudh Pradhan, Gopikant Goswami, Aroonkumar Beesham
In this paper, an attempt is made to construct a Friedmann-Lemaitre-Robertson-Walker model in gravity with a perfect fluid that yields acceleration at late times. We take…
A non-singular bouncing cosmology in gravity
J. K. Singh, Shaily, Akanksha Singh +2
We investigate a bounce realization in the framework of higher order curvature in modified theory of gravity. We perform a detailed analysis of the cosmological paramete…
The Reconstruction of Constant Jerk Parameter with Gravity
Anirudh Pradhan, Gopikant Goswami, Aroonkumar Beesham
In this work, we have developed an FLRW type model of a universe which displays transition from deceleration in the past to the acceleration at the present. For this, we have consi…