Hint of dark matter-dark energy interaction in DESI DR2 and current cosmological dataset?
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2024
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| author | Chakraborty, Amlan Ray, Tulip Das, Subinoy Banerjee, Arka Ganesan, Vidhya |
| author_facet | Chakraborty, Amlan Ray, Tulip Das, Subinoy Banerjee, Arka Ganesan, Vidhya |
| contents | We present new constraints on an interacting dark matter-dark energy scenario motivated by string compactification, where a scalar field adiabatically tracks the minimum of an effective potential sourced by dark matter density. In this study, we focus on the Chameleon dark energy model and numerically solve the Klein-Gordon equation using a shooting algorithm to determine precise initial conditions such that the field rests at effective potential minima today. We perform a comprehensive Markov Chain Monte Carlo (MCMC) analysis using a combination of datasets, including Planck, BAO (SDSS and DESI DR2), Pantheon+, and SH$_0$ES. Our analysis shows a mild preference for a higher non-zero dark sector coupling, compared to earlier works on similar models, for two particular combinations of datasets: (i) Planck + DESI DR2 BAO +.Pantheon+, (ii) Planck + SDSS BAO + Pantheon+ + SH$0$ES. Notably, the inclusion of DESI DR2 and SH$0$ES data increases the inferred interaction strength to $β\sim 0.3$ (68\% C.L.) and yields weak and positive evidence in favor of the model over $Λ$CDM, with $Δχ^2_{\rm min} = -4.75, -6.41$ and $Δ$AIC= $-0.75, -2.41$ respectively. This model remains consistent with a phantom crossing at redshift $z\sim 0.5$, in agreement with the trend indicated by DESI observations. However, due to the settlement of the scalar field at the minima of the effective potential at the present epoch, the effective dark energy equation of state asymptotically approaches $w_{\rm eff}\to -1$. leading to only weak evidence in favor of this model when analyzed using the DESI DR2 dataset. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2403_14247 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Hint of dark matter-dark energy interaction in DESI DR2 and current cosmological dataset? Chakraborty, Amlan Ray, Tulip Das, Subinoy Banerjee, Arka Ganesan, Vidhya Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Phenomenology High Energy Physics - Theory We present new constraints on an interacting dark matter-dark energy scenario motivated by string compactification, where a scalar field adiabatically tracks the minimum of an effective potential sourced by dark matter density. In this study, we focus on the Chameleon dark energy model and numerically solve the Klein-Gordon equation using a shooting algorithm to determine precise initial conditions such that the field rests at effective potential minima today. We perform a comprehensive Markov Chain Monte Carlo (MCMC) analysis using a combination of datasets, including Planck, BAO (SDSS and DESI DR2), Pantheon+, and SH$_0$ES. Our analysis shows a mild preference for a higher non-zero dark sector coupling, compared to earlier works on similar models, for two particular combinations of datasets: (i) Planck + DESI DR2 BAO +.Pantheon+, (ii) Planck + SDSS BAO + Pantheon+ + SH$0$ES. Notably, the inclusion of DESI DR2 and SH$0$ES data increases the inferred interaction strength to $β\sim 0.3$ (68\% C.L.) and yields weak and positive evidence in favor of the model over $Λ$CDM, with $Δχ^2_{\rm min} = -4.75, -6.41$ and $Δ$AIC= $-0.75, -2.41$ respectively. This model remains consistent with a phantom crossing at redshift $z\sim 0.5$, in agreement with the trend indicated by DESI observations. However, due to the settlement of the scalar field at the minima of the effective potential at the present epoch, the effective dark energy equation of state asymptotically approaches $w_{\rm eff}\to -1$. leading to only weak evidence in favor of this model when analyzed using the DESI DR2 dataset. |
| title | Hint of dark matter-dark energy interaction in DESI DR2 and current cosmological dataset? |
| topic | Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Phenomenology High Energy Physics - Theory |
| url | https://arxiv.org/abs/2403.14247 |