Cosmology with Distinct Functions $f$ of the Non-metricity Scalar $Q$ : A Dynamical System Approach
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arXiv
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| Main Authors: | , , , |
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| Format: | Preprint |
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2025
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| _version_ | 1866918072307154944 |
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| author | Biswas, Promila Pal, Subhajit Biswas, Ritabrata Pal, Satyajit |
| author_facet | Biswas, Promila Pal, Subhajit Biswas, Ritabrata Pal, Satyajit |
| contents | Symmetric teleparallel gravity is one among the general relativistic trinity which deals with the non-metricity scalar $Q$. In the Einstein Hilbert action, a function of $Q$ is chosen to be the main contributory part of the Lagrangian and a modified theory of gravity is constructed. In literature, different structures of the function of $Q$ are found which sustain several astrophysical observations like Big Bang nucleosynthesis, late-time cosmic acceleration etc. Autonomous systems for each such models with different $f(Q)$ structures are constructed. Corresponding fixed points and their stability properties are studied. For every case, stable, unstable and saddle-type fixed points are found to exist. These points on the phase portraits are cosmologically analyzed. It is tried to justify which way the corresponding state may lead if the initial state is perturbed. A comparative study of different models is represented. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2506_21646 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Cosmology with Distinct Functions $f$ of the Non-metricity Scalar $Q$ : A Dynamical System Approach Biswas, Promila Pal, Subhajit Biswas, Ritabrata Pal, Satyajit General Relativity and Quantum Cosmology Symmetric teleparallel gravity is one among the general relativistic trinity which deals with the non-metricity scalar $Q$. In the Einstein Hilbert action, a function of $Q$ is chosen to be the main contributory part of the Lagrangian and a modified theory of gravity is constructed. In literature, different structures of the function of $Q$ are found which sustain several astrophysical observations like Big Bang nucleosynthesis, late-time cosmic acceleration etc. Autonomous systems for each such models with different $f(Q)$ structures are constructed. Corresponding fixed points and their stability properties are studied. For every case, stable, unstable and saddle-type fixed points are found to exist. These points on the phase portraits are cosmologically analyzed. It is tried to justify which way the corresponding state may lead if the initial state is perturbed. A comparative study of different models is represented. |
| title | Cosmology with Distinct Functions $f$ of the Non-metricity Scalar $Q$ : A Dynamical System Approach |
| topic | General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2506.21646 |