| Issue |
ITM Web Conf.
Volume 75, 2025
The Second International Conference on Mathematical Analysis and Its Applications (ICONMAA 2024)
|
|
|---|---|---|
| Article Number | 05001 | |
| Number of page(s) | 5 | |
| Section | Mathematical Physics | |
| DOI | https://doi.org/10.1051/itmconf/20257505001 | |
| Published online | 21 February 2025 | |
Stability of Fluctating Baby-Skyrme Brane
1 Theoretical High Energy Physics Research Division, Faculty of Mathematics and Natural Sciences, Institut Teknologi Bandung, Jl. Ganesha no. 10, Bandung, 40132, Indonesia
2 Research Center for Quantum Physics, National Research and Innovation Agency (BRIN), Kompleks PUSPIPTEK Serpong, Tangerang Selatan, 15310, Indonesia
* e-mail: emir002@brin.go.id
** e-mail: bobby@itb.ac.id
*** e-mail: agussuroso@itb.ac.id
**** e-mail: ardi002@brin.go.id
This work studies the stability of fluctuating Baby-Skyrme brane as a model for early-time cosmology recently introduced in [1]. The dynamical system consists of two dynamical quantities (ϕ, H) with two differential equations and one constraint. The solutions can be realized as a family of curves on a surface in ℝ3. We found that there exist stable solutions provided that the physical parameters (α, σ, k) satisfy certain conditions that are deduced from the linear stability conditions near the critical points.
© The Authors, published by EDP Sciences, 2025
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.