New Horizons in Mathematical Physics

Download PDF (480.2 KB) PP. 37 - 43 Pub. Date: September 1, 2018

DOI: 10.22606/nhmp.2018.23001

• Shri Ram^*
  Dept. of Math. Sci., Indian Institute of Technology Varanasi -2210 05, India
• Surendra K. Singh
  Pt. Ramadhar J. Tiwari College of Polytechnic, Mahur Kalan, Chandauli, 221115, India
• M. K. Verma
  Dept. of Math. Sci., Indian Institute of Technology Varanasi -2210 05, India

Einstein’s field equations in f(R, T) gravity theory in the presence of quark and strange quark matter are considered for a plane symmetric space-time. We have obtained exact solutions of the field equations by assuming a special form of Hubble parameter that yield a time-varying deceleration parameter. The physical behaviors of the cosmological model are discussed.

Plane symmetric Space-Time; Quark and Strange Quark Matter; f(R, T) Gravity Theory; Time-Dependent Deceleration Parameter.

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