Anisotropic Quintessence Strange Stars in f(T) Gravity with Modified Chaplygin Gas

In this paper, we study the existence of strange star in the background of f (T) modified gravity where T is a scalar torsion. In KB metric space, we derive the equations of motion using anisotropic property within the spherically strange star with modified chaplygin gas in the framework of modified f (T) gravity. Then we obtain many physical quantities to describe the physical status such as anisotropic behavior, energy conditions and stability. By the matching condition, we calculate the unknown parameters to evaluate the numerical values of mass, surface redshift etc. from our model to make comparison with the observational data.


Introduction
In modern cosmology, cosmic acceleration is an interesting discovery. The observation of type Ia supernovae (SNeIa) together with the cosmic microwave background (CMB), large scale structure surveys (LSS), and Wilkinson Microwave Anisotropy Probe (WMAP) [1][2][3][4] ensures the presence of an exotic energy component dominating our universe which is entitled as dark energy (DE) having equation of state = with strong negative pressure. For accelerating expansion must satisfy the range < −1/3. If −1 < < −1/3 then it belongs to quintessence phase and if < −1, then it belongs to phantom regime. In particular, when = −1 ⇒ = − then the equation of state of the interior region of a Gravastar (gravitationally vacuum condense star) is described in [ -]. There are many investigations of this cosmic expansion and nature of DE based on different ways. These efforts can be classified as follows: (i) to modify the entire cosmic energy by including new components of DE and (ii) to modify Einstein-Hilbert action to get different types of modified theories of gravity such as ( ) gravity [11,12], being the Ricci scalar; ( ) gravity [13], being the torsion; ( , ) gravity [14], Gauss-Bonnet gravity, i.e., ( ) modified gravity [15], etc. Here we assume only ( ) gravity theory.
Since general relativity is similar to ( ), this theory could be a substitute form of the generalized general relativity, named as ( ) theory of gravity. The teleparallel equivalence of gravity (TEGR) gives the concept of this theory. There is defined Riemann-Cartan space-time together with Weitzenbock connections rather than Levi-Civita connections in ( ) theory. Here, nonzero torsion and zero curvature appear in the background space-time. Einstein gives this definition of space-time to give an idea of gravitation related to tetrad and torsion. Instead of metric field, tetrad field takes an important role in dynamic field in TEGR.
In ( ) gravity, equations of motions are second-order differential equations like GR whereas equations of motion are fourth-order in ( ) gravity. So, the former one is more convenient than the latter one. Recently, a wide interest has been seen to study the ( ) gravity [16][17][18][19][20]. There is no doubt of excellence of ( ) theory to explain the cosmic acceleration and analysis on large scale (clustering of galaxies) [21]. But GR must be a fantabulous agreement with solar system test and pulsar observation [22].
In theoretical astrophysics, ( ) version of BTZ black hole solutions has been calculated as ( ) theory was supported for examining the effects of ( ) models in 3 dimensions [23]. Later on [ ], violation of Lorentz invariance made the first violation of black hole thermodynamics < 1. A study of strange star with MIT bag model in the framework of ( ) gravity has been done by Abbas et al. [ ]. Here, our main motivation of this paper is to study the anisotropic strange star models in the framework of ( ) gravity with diagonal tetrad in presence of electric field and modified Chaplygin gas. In Section 2, we give a brief idea of ( ) gravity. In Section , we study anisotropic quintessence strange star in ( ) gravity with the help of modified Chaplygin gas. In Section , we analyze many physical phenomenon of this whole system. By matching of two metrics, the unknown constants are found out. We also make stability analysis. In Section , we calculate the mass function, compactness, and surface redshi function from our model to compare with observational data and finally, in Section , we give the summarization.

( ) Gravity: Fundamentals
In this section, we briefly overview the basics of ( ) gravity. We define the torsion and the con-torsion tensor as follows [51]: and the components of the tensor ] are defined as one can write the torsion scalar as Now, one can define the modified teleparallel action by replacing with a function of , in analogy to ( ) gravity [52,53], as follows: where we used = = 1 and Φ is matter fields. The ordinary matter is an anisotropic fluid so that the energy-momentum tensor is given by where is the four-velocity, V is radial four vectors, is the energy density, is the radial pressure, and is transverse pressure. Further, the energy-momentum tensor for electromagnetic field is given by where ] is the Maxwell field tensor defined as and Φ is the four potential.

Anisotropic Strange Quintessence Star in ( ) Gravity
We consider the KB metric [42] describing the interior spacetime of a strange star where we assume ( ) and ( ) are Advances in High Energy Physics where , , and are arbitrary constants. For the charged fluid source with density ( ), radial pressure ( ), and tangential pressure ( ), the Einstein-Maxwell (EM) equations reduce to the form ( = = 1) [51] where the prime denotes the derivative with respect to the radial coordinate . Now the equations of motion for anisotropic fluid are [51] 4 4 where ( ) is the total charge within a sphere of radius . We introduce the modified Chaplygin gas (MCG) having equation of state [54] = − (18) where , , and are free parameters of the model. From (16) we get where and 1 are integration constants and we assume 1 = 0 for simple case. Now from (10), (11), (13), (14), (18), and (19) we obtain the equation in Here we take = 1; then (20) reduces to the quadratic equation in Solving this equation we get the value of energy density as = (2 + 3 + 3 ) + √ 256 2 2 3 (1 + ) + (2 + 3 + 3 ) and corresponding components are Advances in High Energy Physics Now from Figures 1 and 2, we conclude that anisotropic strange star in ( ) gravity with modified Chaplygin gas acts as a dark energy candidate due to > 0, < 0. Again with the help of Figures 3 and 4, we notice that the equation of state = / lies between −1/3 and −1; i.e., the corresponding model belongs to quintessence phase not phantom phase.
The amount of net charge inside a sphere having radius r is

Physical Analysis
The central density 0 and central radial pressure 0 are given by and In this section, we investigate the nature of the anisotropic compact star as the following subsection.

Anisotropic
Behavior. Now we take the derivatives of (22) and (23) with respect to , given by Advances in High Energy Physics     Advances in High Energy Physics      Now we present the evolution of / and / by Figures 6 and 7. Figure 6 shows that / decreases keeping / < 0 (as energy density decreases) and Figure 7 shows that / decreases keeping d / < 0 (as for dark energy pressure is negatively very high; i.e., pressure decreases negatively). From Figures 6, 7, 8, and 9 we notice that, at = 1.46, From Figure 10, we notice that Δ > 0 for = 1, −6 which imply that the anisotropic stress is outwardly directed and there exists repulsive gravitational force for the strange star and for = −15, Δ < 0 in somewhere implying the existence of attractive gravitational force and Δ > 0 in the remaining part implying the existence of repulsive gravitational force of the strange star. Figure 11 shows that 2 is decreasing with the increment of the radial coordinate.

Energy Conditions.
Energy conditions are very useful tools to discuss cosmological geometry in general relativity and modified gravity [10,48,51]. These include null energy condition (NEC), weak energy condition (WEC), and strong energy condition (SEC), given as Figures 6, 7, 8, and 9 represent the plots of / , / , 2 / 2 , and 2 / 2 with respect to to show the maximality of density and radial pressure at = 1.46 of the strange star taking = 1, = 7, = 0.1, = 9, and = 10. Figure 10 represents the plots of Δ with respect to to show the presence of repulsive and attractive force of the strange star and Figure 11 represents the plot of 2 with respect to taking = 10, = 1, = 10, = 2, and = 1.
From Figures 12, 4, 13, and 14, we observe that the interior of our proposed strange star model satisfies all energy conditions.
The continuity of the metric components , , and / at the boundary surface = yields where − and + indicate interior and exterior solutions. Now, using (36) and the metrics (9) and (35), we have For the values of and for a strange stars, we compute the constants , , and , specified as in Table 1.

4.4.
Stability. Now we calculate the two sound speed squares V 2 , V 2 for the radial and transverse coordinate, respectively. Herrera [55] introduced cracking concept and developed a new technique to examine potential stability for the matter. If we investigate the sign of the difference V 2 − V 2 then we can conclude whether our strange star is potential stable or not; i.e., if the radial speed sound is greater than the transverse speed sound, then there exists potentially stable region; otherwise, the region will be potentially unstable [10,47,49,51]. It is clear from Figures and that 0 < V 2 ≤ 1 and 0 < V 2 ≤ 1 always within the stellar objects.
From Figure 17, we see that the corresponding difference is    Advances in High Energy Physics 9 Table 1: The values of , , and have been obtained using (37).

Compact Stars
1808. 4   negative which means the radial speed sound is greater than the transverse speed sound which implies that our proposed strange star model is potentially stable in the framework of ( ) gravity. Again Figure shows Figures 12,13, and 14 represent the plots to understand the validation of the energy conditions taking = 10, = 1, = 10, = 2, and = 1.

Mass Function and Compactness.
The mass function within the radius is defined as [10] ( ) = ∫ From Figure 19, we have seen that at origin the mass function is regular (i.e., ( ) → 0 when → 0) and monotonic increasing with respect to radius ( ). We have also evaluated the values of mass for a few strange stars from our model to compare these values with observational data (see Table 2).
The compactness of the star is defined by ( ) [10] in the form of We have plotted the corresponding function given by Figure 20.

Relation between Mass and Radius.
In this section we discuss the mass radius relation of the strange stars. From [57], twice the maximum allowable ratio of mass to the radius for an astrophysical object is always less than 8/9 (2 / < 8/9) whereas the factor / is called "compactification factor". From Table 3, we find that the calculated values corresponding to our model lie in the expected range [34]. Compactification factor for strange star always lies between 1/4 and 1/2. The calculated values of the compactification factor of the strange stars from our model are compatible with the condition (see Table 3).

Surface Redshift.
The redshift function can be defined as [10,47,49,51] where ( ) has been obtained from (38). According to Bohmer and Harko, the surface redshift should be ≤ 5 for       an anisotropic star in the presence of a cosmological constant [58]. We calculate the maximum surface redshift from our model in Table 3. Now, it is clear that our model for strange stars obeys the relation ≤ 5 though the cosmological constant is absent in our model which is quite reasonable.

Discussions
This paper has given out the anisotropic strange star model in ( ) gravity with modified Chaplygin gas. Using the diagonal tetrad field we have obtained the equations of motion where we have solved the unknown function ( ) as + 1 , and 1 being constants. Then we have solved the differential equation of energy density from where we have found the value of energy density (22) of it. With the help of this energy density, we have found out radial pressure ensuring this model as a quintessence dark energy candidate from Figures  1, 2, 3, and 4. We have also noticed that both the energy density ( ) and radial pressure ( ) are monotonic decreasing function with respect to and they have maximum value at = 1.46 by Figures 6-9. Figure 5 shows that the transverse pressure is decreasing with the rise of . We have calculated anisotropic factor to see whether there exists gravitational attractive force or repulsive force for the strange star and we have studied from Figure 10 that there exists attractive force as well as repulsive gravitational force with different values of . Here, the square of energy is monotonic decreasing with the increment of radial coordinate given by Figure 11. From Figures 12,4,13, and 14 we have concluded that all energy conditions are satisfied for our proposed model.
Using matching condition, the unknown parameters , , and have been calculated for the different strange stars from our model which is given by Table 1. By stability analysis given on the basic of Figures 15-18, we have observed that 0 < V 2 , V 2 ≤ 1, V 2 > V 2 , and |V 2 − V 2 | ≤ 1 always. Finally, we have ensured that our model is potentially stable.
In Table 2, with the help of energy density (22) and radial pressure (23) we have calculated the numerical values of the mass of the different strange stars from our model to show the closeness of these values with the observational data. Also, we have obtained the values of central and surface density and central pressure for the above-mentioned strange stars from our model which have been calculated in Table 2. From Table 3, we have observed that twice the compactification factor are always less than < 8/9 and maximum values of the surface redshift function are always less than 5. So, our proposed model is completely rational. Figures 19, 20, and 21 represent the plots of mass function, compactness, and surface redshift function taking the values of , , and from Table 1 and = 2 and = 1.

Data Availability
No data were used to support this study.

Conflicts of Interest
The authors declare that they have no conflicts of interest.