Here, we mainly focused on the reconstruction of the tachyon scalar eld dark energy prescription by making use of the variable generalized Chaplygin gas (VGCG) dark energy model in the four-dimensional (4D) spatially at Friedmann-Robertson-Walker (FRW) framework.
📌 3 Key Takeaways
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Objective & Hypothesis:A large number of scalar eld ideas have been introduced in literature in order to discuss the speedy expansion nature of our universe.
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Key Findings & Data:Fundamental particle physics theories can yield various scalar eld descriptions, but they do not dene its self-interacting potential exactly due to the complexity of corresponding equations.
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Conclusion & Impact:Here, we mainly focused on the reconstruction of the tachyon scalar eld dark energy prescription by making use of the variable generalized Chaplygin gas (VGCG) dark energy model in the four-dimensional (4D) spatially at Friedmann-Robertson-Walker (FRW) framework.
🔬Design:Modeling & Simulation
📍Scope:Comprehensive Sample
⚙️Variables:Cosmology · Dark Energy · Scalar Field
Abstract
A large number of scalar eld ideas have been introduced in literature in order to discuss the speedy expansion nature of our universe. Scalar eld denitions naturally come forward in particle physics. Fundamental particle physics theories can yield various scalar eld descriptions, but they do not dene its self-interacting potential exactly due to the complexity of corresponding equations. Here, we mainly focused on the reconstruction of the tachyon scalar eld dark energy prescription by making use of the variable generalized Chaplygin gas (VGCG) dark energy model in the four-dimensional (4D) spatially at Friedmann-Robertson-Walker (FRW) framework.
SALTI, M., KORUNUR, M., SOGUT, K., AYDOĞDU, O. (2019). VARIABLE GENERALIZED CHAPLYGIN GAS AS A SCALAR FIELD DARK ENERGY MODEL. Journal of Universal Mathematics, Cilt: 2 - Sayı: 1, 98–102. https://ajindex.com/articles/782235
S. Perlmutter, et al., Measurements of Omega and Lambda from 42 High-Redshift Supernovae, Astrophys. J., 517, 565 (1999).C.L. Bennet, et al., First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results, Astrophys. J. Suppl., 148, 1 (2003). M. Tegmark, et al., Cosmological parameters from SDSS and WMAP, Phys. Rev. D, 69, 103501(2004). A.W. Allen, et al., Constraints on dark energy from Chandra observations of the largest relaxed galaxy clusters, Mon. Not. R. Astron. Soc., 353, 457 (2004).P.A.R. Ade, et al., Planck 2013 results - XII. Component separation, A&A 571, A12 (2014).P.A.R. Ade, et al., Planck 2015 results - XIII. Cosmological parameters, A&A 594, A13 (2016).M.F. Wondrak, The Cosmological Constant and its Problems: A Review of Gravitational Aether, e-Print: gr-qc/1705.06294 V. Sahni, Dark matter and dark energy, Lect. Notes Phys., 653, 141-180 (2004).
E.J. Copeland, M. Sami and S. Tsujikawa, Dynamics of dark energy, Int. J. Mod. Phys. D,15, 1753 (2006).
R.R. Caldwell, A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state, Phys. Lett. B, 545, 23-29 (2002).B. Feng, X. L. Wang and X. M. Zhang, Dark Energy Constraints from the Cosmic Age and Supernova, Phys. Lett. B, 607, 35 (2005).T. Chiba, T. Okabe and M. Yamaguchi, Kinetically driven quintessence, Phys. Rev. D, 62, 023511 (2000).A. Yu. Kamenshchik, U. Moschella and V. Pasquier, An alternative to quintessence, Phys. Lett. B, 511, 265 (2001).J. Christensen-Dalsgard, Lecture Notes on Stellar Structure and Evolution, Aarhus Univ. Press, Aarhus, p.13 (2004).M. Salti, O. Aydogdu, H. Yanar and K. Sogut, Variable generalized Chaplygin gas in a 5D cosmology, Annals of Physics, 390, 131-142 (2018).
M. Askin, M. Salti and O. Aydogdu, Cosmology via thermodynamics of Polytropic gas, Mod. Phys. Lett. A, Vol.32, No.32, 1750177 (2017).
B. Boisseau, G. Esposito-Farese, D. Polarski and A. A. Starobinsky, Reconstruction of a scalar-tensor theory of gravity in an accelerating universe, Phys. Rev. Lett., 85, 2236 (2000).
S. Capozziello, Curvature Quintessence, Int. J. Mod. Phys. D, 11, 483 (2002). V. Faraoni, f(R)-gravity: Successes and challenges, XVIII Congresso SIGRAV General Relativity and Gravitational Physics, Cosenza, 2225 September (2008).
S. Capozziello, R. Cianci, C. Stornaiolo and S. Vignolo, f(R) Cosmology with torsion, Phys. Scr., 78, 065010 (2008).
H. Abedi and M. Salti, Multiple field modifed gravity and loca