Saved in:
| Main Author: | |
|---|---|
| Format: | Preprint |
| Published: |
2024
|
| Subjects: | |
| Online Access: | https://arxiv.org/abs/2412.20551 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866911320832475136 |
|---|---|
| author | Neomenko, Roman |
| author_facet | Neomenko, Roman |
| contents | In this work the observational constraints on interaction coupling parameter between dynamical dark energy and cold dark matter were obtained using CMB, BAO and SN Ia data. The dark energy in considered models is dynamical and evolution of its equation of state parameter depends on dark coupling and internal properties of the dark energy. Such model is believed to be more physically consistent than models of interacting dark energy considered in previous works. Constraints were made for three types of interaction. The first two are the types which are often considered in other works on interacting dark energy. The third type has the non-linear dependence on densities of dark components and is studied for the first time. Observational constraints on Hubble constant $H_{0}$ for the first two models are in strong disagreement with so called local measurements of $H_{0}$. And the third model is in better agreement with local measurements than $Λ$CDM model. Also for the last non-linear model existence of non-zero interaction was found at greater than $1σ$ significance level. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2412_20551 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Constraints on the interaction strength in the model of interacting dynamical dark energy with linear and non-linear interacting terms Neomenko, Roman Cosmology and Nongalactic Astrophysics In this work the observational constraints on interaction coupling parameter between dynamical dark energy and cold dark matter were obtained using CMB, BAO and SN Ia data. The dark energy in considered models is dynamical and evolution of its equation of state parameter depends on dark coupling and internal properties of the dark energy. Such model is believed to be more physically consistent than models of interacting dark energy considered in previous works. Constraints were made for three types of interaction. The first two are the types which are often considered in other works on interacting dark energy. The third type has the non-linear dependence on densities of dark components and is studied for the first time. Observational constraints on Hubble constant $H_{0}$ for the first two models are in strong disagreement with so called local measurements of $H_{0}$. And the third model is in better agreement with local measurements than $Λ$CDM model. Also for the last non-linear model existence of non-zero interaction was found at greater than $1σ$ significance level. |
| title | Constraints on the interaction strength in the model of interacting dynamical dark energy with linear and non-linear interacting terms |
| topic | Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2412.20551 |