Best Paper Award
| Zanyar Ebrahimi | |
|---|---|
| Affiliation | Research Institute For Astronomy & Astrophysics Of Maragha |
| Country | Iran |
| Article Title | Structure formation in a non-canonical scalar field model of clustering dark energy |
| Scopus ID | 55759620100 |
| Article Type | Research Article |
| Subject Area | Physics and Astronomy |
| Reference Count | 105 |
| Award Category | Best Paper Award |
| Event | International Research Excellence and Best Paper Awards |
| ORCID | 0000-0003-2548-2678 |
The Best Paper Award recognizes the scholarly contribution of Zanyar Ebrahimi for the article titled Structure formation in a non-canonical scalar field model of clustering dark energy. Published within the field of Physics and Astronomy in 2026, the study investigates theoretical aspects of cosmic structure formation under alternative dark energy frameworks. The research contributes to ongoing discussions regarding cosmological evolution, matter clustering, and scalar field dynamics while demonstrating methodological rigor and scientific relevance.[1]
Abstract
This award-winning research examines the formation and evolution of cosmic structures within a non-canonical scalar field framework describing clustering dark energy. The study explores how modifications to conventional dark energy assumptions influence the growth of density perturbations and large-scale matter distributions throughout cosmic history. Through theoretical modeling and cosmological analysis, the work evaluates the compatibility of alternative scalar field dynamics with observed structure formation patterns. The findings provide valuable insight into dark energy behavior, the evolution of gravitational instabilities, and the broader understanding of cosmological expansion, contributing to contemporary investigations of the universe’s large-scale structure and theoretical cosmology.[2]
Keywords
Dark Energy, Scalar Field Cosmology, Structure Formation, Clustering Dark Energy, Cosmological Perturbations, Theoretical Astrophysics, Large Scale Structure, Physics and Astronomy.
Introduction
Dark energy remains one of the most significant unresolved questions in modern cosmology. Understanding how it influences the growth of galaxies, clusters, and large-scale structures is essential for explaining the universe’s accelerated expansion. Alternative scalar field models offer theoretical possibilities beyond standard cosmological assumptions and continue to attract scientific interest.[3]
Research Profile
Zanyar Ebrahimi is affiliated with the Research Institute For Astronomy & Astrophysics Of Maragha and has contributed to studies in cosmology, astrophysics, and theoretical physics. The recognized article reflects a research focus on dark energy dynamics, cosmological perturbation theory, and mechanisms governing structure formation in the evolving universe.[1]
Scientific Background
Conventional cosmological models often represent dark energy as a cosmological constant. However, scalar field approaches introduce dynamic properties that may better explain observational phenomena. Non-canonical scalar fields modify kinetic terms and can alter the behavior of perturbations, thereby affecting matter clustering and the development of large-scale cosmic structures over time.[4]
Methodology
The research employs theoretical cosmological modeling, perturbation analysis, and comparative evaluation of scalar field dynamics. Mathematical formulations are used to investigate clustering behavior and structure growth under non-canonical conditions. Predictions generated by the model are examined against accepted cosmological principles to assess consistency and scientific relevance.[2]
Key Findings
The study indicates that non-canonical scalar field models can influence matter perturbation growth and produce distinctive clustering characteristics. Results suggest that dark energy dynamics may play a more active role in structure formation than traditionally assumed. These outcomes provide additional theoretical pathways for interpreting observations related to cosmic expansion and matter distribution.[2]
Scientific Contributions
This research contributes to theoretical astrophysics by extending investigations into alternative dark energy models and their cosmological implications. The work enhances understanding of clustering dark energy, supports the development of advanced cosmological frameworks, and offers valuable perspectives for future observational and theoretical studies in large-scale structure formation.[5]
Conclusion
The Best Paper Award acknowledges a significant scholarly contribution to the study of cosmological structure formation and dark energy theory. By examining non-canonical scalar field dynamics within a clustering dark energy framework, the research expands theoretical understanding and encourages further exploration of fundamental mechanisms shaping the evolution of the universe.[2]
External Links
References
- Elsevier. (2026). Structure formation in a non-canonical scalar field model of clustering dark energy. Journal of High Energy Astrophysics.
https://doi.org/10.1016/j.jheap.2025.100496 - ScienceDirect. (2026). Journal of High Energy Astrophysics – Research Publication Record.
https://www.sciencedirect.com/journal/journal-of-high-energy-astrophysics - General Relativity and Quantum Cosmology. (2025). Structure formation in a non-canonical scalar field model of clustering dark energy.
https://doi.org/10.48550/arXiv.2510.16589 - International Research Excellence and Best Paper Awards. (2026). Best Paper Award Recognition Program.
https://bestpaperawards.com/ - Elsevier. (n.d.). Scopus author details: Zanyar Ebrahimi, Author ID 55759620100. Scopus.
https://www.scopus.com/authid/detail.uri?authorId=55759620100