Cosmological Model with Strange Quark Matter Attached to Cosmic String for Axially Symmetric Space-Time

2012 ◽  
Vol 51 (6) ◽  
pp. 1881-1888 ◽  
Author(s):  
S. D. Katore ◽  
A. Y. Shaikh
2005 ◽  
Vol 14 (08) ◽  
pp. 1365-1372 ◽  
Author(s):  
İLHAMİ YAVUZ ◽  
İHSAN YILMAZ ◽  
HÜSNÜ BAYSAL

In this paper, we have examined charged strange quark matter attached to the string cloud in the spherical symmetric space–time admitting one-parameter group of conformal motions. For this purpose, we have solved Einstein's field equations for spherical symmetric space–time with strange quark matter attached to the string cloud via conformal motions. Also, we have discussed the features of the obtained solutions.


2021 ◽  
Vol 9 (04) ◽  
pp. 264-271
Author(s):  
Samadhan L. Munde ◽  

In this paper,Kaluza-Klein space-time with quark and strange quark matter in gravity has been considered. The general solutions of the field equations of Kaluza-Klein space-time have been obtained under the assumption of constant deceleration parameter. The physical and geometrical aspects of the model are also discussed in details.


2014 ◽  
Vol 69 (1-2) ◽  
pp. 90-96 ◽  
Author(s):  
Namrata Jain ◽  
Shyamsunder S. Bhoga ◽  
Gowardhan S. Khadekar

In this paper, exact solutions of the Einstein field equations of the Kaluza-Klein cosmological model have been obtained in the presence of strange quark matter. We have considered the timevarying cosmological constant Λ as Λ = αH2 + βR-2, where α and β are free parameters. The solutions are obtained with the help of the equation of state for strange quark matter as per the Bag model, i.e. quark pressure p = 1/3(ρ - 4BC), where BC is Bag’s constant. We also discussed the physical implications of the solutions obtained for the model for different types of universes.


Open Physics ◽  
2015 ◽  
Vol 13 (1) ◽  
Author(s):  
Kishor S. Adhav ◽  
Abhijit S. Bansod ◽  
Samadhan L. Munde

AbstractIn this paper we have studied the Kantowski- Sachs cosmological model with the quark and strange quark matter in the f (R) theory of gravity. The general solutions of the field equations are obtained by assuming the physical condition shear scalar σ is proportional to scalar expansion θ, which leads to the relation B = An between metric coefficients B and A. The physical and geometrical aspects of the model are also discussed.


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