Article
Kyungpook Mathematical Journal 2018; 58(2): 361-375
Published online June 23, 2018
Copyright © Kyungpook Mathematical Journal.
Super Quasi-Einstein Manifolds with Applications to General Relativity
Sahanous Mallick
Department of Mathematics, Chakdaha College, P. O.-Chakdaha, Dist-Nadia, West Bengal, India, e-mail: sahanousmallick@gmail.com
Received: September 27, 2017; Accepted: March 17, 2018
Abstract
- Abstract
- 1. Introduction
- 2.
S (QE )n admitting Quasi-conformal Curvature Tensor - 3. The Generators
U andV as Killing Vector Fields - 4. The Generators
U andV as Concurrent Vector Fields - 5. The Generators
U andV as Recurrent Vector Fields - 6.
S (QE )4 Spacetimes - 7. Example of a
S (QE )4 Spacetimes - Acknowledgements
- References
The object of the present paper is to study super quasi-Einstein manifolds. Some geometric properties of super quasi-Einstein manifolds have been studied. We also discuss
Keywords: super quasi-Einstein manifolds, concurrent vector field, energy momentum tensor, Einstein's field equation, space-matter tensor
1. Introduction
- Abstract
- 1. Introduction
- 2.
S (QE )n admitting Quasi-conformal Curvature Tensor - 3. The Generators
U andV as Killing Vector Fields - 4. The Generators
U andV as Concurrent Vector Fields - 5. The Generators
U andV as Recurrent Vector Fields - 6.
S (QE )4 Spacetimes - 7. Example of a
S (QE )4 Spacetimes - Acknowledgements
- References
A Riemannian or semi-Riemannian manifold (
holds on M, where
where
for all vector fields
A non-flat Riemannian or semi-Riemannian manifold (
It is to be noted that Chaki and Maity [9] also introduced the notoin of quasi-Einstein manifolds in a different way. They have taken a, b are scalars and the vector field U metrically equivalent to the 1-form A as a unit vector field. Such an n-dimensional manifold is denoted by (
Quasi-Einstein manifolds arose during the study of exact solutions of the Einstein field equations as well as during considerations of quasi-umbilical hypersurfaces of semi-Euclidean spaces. For instance, the Robertson-Walker spacetimes are quasi-Einstein manifolds. So quasi-Einstein manifolds have some importance in the general theory of relativity.
Quasi-Einstein manifolds have been generalized by several authors in several ways such as generalized quasi-Einstein manifolds [7, 14, 40], super quasi-Einstein manifolds [8, 21, 34] and many others.
As a generalization of quasi-Einstein manifold Chaki introduced the notion of a super quasi-Einstein manifold in [8]. According to him a non-flat Riemannian or semi-Riemannian manifold (
where
for all
A Riemannian or semi-Riemannian manifold of quasi-constant curvature was given by Chen and Yano [10] as a conformally flat manifold with the curvature tensor
where
for all
It can be easily seen that if the curvature tensor
Subsequently Chaki [8] generalized the notion of (
A non-flat Riemannian or semi-Riemannian manifold (
where
The notion of quasi-conformal curvature tensor was given by Yano and Sawaki [43] and is defined as follows:
where
If
The spacetime of general relativity and cosmology is regarded as a connected 4-dimensional semi-Riemannian manifold (
The present paper is organized as follows:
After introduction in Section 2 we study
2. S (QE )n admitting Quasi-conformal Curvature Tensor
- Abstract
- 1. Introduction
- 2.
S (QE )n admitting Quasi-conformal Curvature Tensor - 3. The Generators
U andV as Killing Vector Fields - 4. The Generators
U andV as Concurrent Vector Fields - 5. The Generators
U andV as Recurrent Vector Fields - 6.
S (QE )4 Spacetimes - 7. Example of a
S (QE )4 Spacetimes - Acknowledgements
- References
A
Using (
where
In virtue of (
Theorem 2.1
Now we look for sufficient condition in order that a
In a
which implies that the scalar curvature
We know that (
since
Contracting (
Imposing the condition that the generators
and
Therefore from (
Thus we can state the following:
Theorem 2.1
3. The Generators U and V as Killing Vector Fields
- Abstract
- 1. Introduction
- 2.
S (QE )n admitting Quasi-conformal Curvature Tensor - 3. The Generators
U andV as Killing Vector Fields - 4. The Generators
U andV as Concurrent Vector Fields - 5. The Generators
U andV as Recurrent Vector Fields - 6.
S (QE )4 Spacetimes - 7. Example of a
S (QE )4 Spacetimes - Acknowledgements
- References
In this section let us consider the generators
and
where
From (
and
Since
and
for all
Similarly, we have
for all
We also assume that the associated scalars are constants. Then from (
Using (
By virtue of (
Thus we can state the following theorem:
Theorem 3.1
4. The Generators U and V as Concurrent Vector Fields
- Abstract
- 1. Introduction
- 2.
S (QE )n admitting Quasi-conformal Curvature Tensor - 3. The Generators
U andV as Killing Vector Fields - 4. The Generators
U andV as Concurrent Vector Fields - 5. The Generators
U andV as Recurrent Vector Fields - 6.
S (QE )4 Spacetimes - 7. Example of a
S (QE )4 Spacetimes - Acknowledgements
- References
A vector field
where
In this section we consider the vector fields
and
where
Now using (
Contracting (
where
Now contracting (
Thus,
Since
Thus the manifold reduces to a pseudo quasi-Einstein manifold. Hence we can state the following:
Theorem 4.1
5. The Generators U and V as Recurrent Vector Fields
- Abstract
- 1. Introduction
- 2.
S (QE )n admitting Quasi-conformal Curvature Tensor - 3. The Generators
U andV as Killing Vector Fields - 4. The Generators
U andV as Concurrent Vector Fields - 5. The Generators
U andV as Recurrent Vector Fields - 6.
S (QE )4 Spacetimes - 7. Example of a
S (QE )4 Spacetimes - Acknowledgements
- References
A vector fields
where
In this section we suppose that the generators
and
where λ and
A non-flat Riemannian or semi-Riemannian manifold (
where
Now, using (
We assume that the 1-forms λ and
for all Z. Then we obtain from (
Using (
where
Thus we can state the following:
Theorem 5.1
6. S (QE )4 Spacetimes
- Abstract
- 1. Introduction
- 2.
S (QE )n admitting Quasi-conformal Curvature Tensor - 3. The Generators
U andV as Killing Vector Fields - 4. The Generators
U andV as Concurrent Vector Fields - 5. The Generators
U andV as Recurrent Vector Fields - 6.
S (QE )4 Spacetimes - 7. Example of a
S (QE )4 Spacetimes - Acknowledgements
- References
In a smooth manifold (
where
for all
where
In this section we first study
If
The Einstein’s field equation without cosmological constant is given by [32, 33]
where
Now using (
In virtue of (
Thus we can state the following:
Theorem 6.1
But it has been proved by Shaikh[39] that if a viscous fluid pseudo quasi-Einstein spacetime obeys Einstein’s field equation with a cosmological constant, then none of the energy density and isotropic pressure of the fluid can be a constant.
In view of Theorem 4.1 and the result of Shaikh leads to the following theorem:
Theorem 6.2
This result has significant agreement with the recent day observational truth that energy density and isotropic pressure can not be a constant. Here we discuss the form of energy momentum tensor [27] as follows:
where
Hence we conclude that if the associated vector fields of a
7. Example of a S (QE )4 Spacetimes
- Abstract
- 1. Introduction
- 2.
S (QE )n admitting Quasi-conformal Curvature Tensor - 3. The Generators
U andV as Killing Vector Fields - 4. The Generators
U andV as Concurrent Vector Fields - 5. The Generators
U andV as Recurrent Vector Fields - 6.
S (QE )4 Spacetimes - 7. Example of a
S (QE )4 Spacetimes - Acknowledgements
- References
In this section we prove the existence of a
We consider a Lorentzian manifold (
where
The only non-vanishing components of the Christoffel symbols, the curvature tensor and the Ricci tensor are
We take the scalars
We choose the 1-forms as follows:
and
at any point
We take the associated tensor as follows:
at any point
It can be easily prove that the
We shall now show that the 1-forms are unit and orthogonal. Here,
So, the manifold under consideration is a
Acknowledgements
- Abstract
- 1. Introduction
- 2.
S (QE )n admitting Quasi-conformal Curvature Tensor - 3. The Generators
U andV as Killing Vector Fields - 4. The Generators
U andV as Concurrent Vector Fields - 5. The Generators
U andV as Recurrent Vector Fields - 6.
S (QE )4 Spacetimes - 7. Example of a
S (QE )4 Spacetimes - Acknowledgements
- References
The author is thankful to the referee for his/her critical remarks and constructive suggestions towards the improvement of the paper.
References
- Abstract
- 1. Introduction
- 2.
S (QE )n admitting Quasi-conformal Curvature Tensor - 3. The Generators
U andV as Killing Vector Fields - 4. The Generators
U andV as Concurrent Vector Fields - 5. The Generators
U andV as Recurrent Vector Fields - 6.
S (QE )4 Spacetimes - 7. Example of a
S (QE )4 Spacetimes - Acknowledgements
- References
- Ahsan, Z (1996). A symmetry property of the spacetime of general relativity in terms of the space-matter tensor. Brazilian J Phys. 26, 572-576.
- Ahsan, Z, and Siddiqui, SA (2010). On the divergence of the space-matter tensor in general relativity. Adv Stud Theor Phys. 4, 543-556.
- Amur, K, and Maralabhavi, YB (1977). On quasi-conformally flat spaces. Tensor (NS). 31, 194-198.
- Beem, JK, and Ehrlich, PE (1981). Global Lorentzian geometry. New York: Marcel Dekker
- Bejan, C-L (2007). Characterization of quasi-Einstein manifolds. An Stiint Univ Al I Cuza Iasi Mat (NS). 53, 67-72.
- Besse, AL (1987). Einstein manifolds. Ergeb Math Grenzgeb, 3 Folge, Bd 10. Berlin, Heidelberg, New York: Springer-Verlag
- Chaki, MC (2001). On generalized quasi-Einstein manifolds. Publ Math Debrecen. 58, 683-691.
- Chaki, MC (2004). On super quasi-Einstein manifolds. Publ Math Debrecen. 64, 481-488.
- Chaki, MC, and Maity, RK (2000). On quasi Einstein manifolds. Publ Math Debrecen. 57, 297-306.
- Chen, BY, and Yano, K (1973). Special conformally flat spaces and canal hypersurfaces. Tohoku Math J. 25, 177-184.
- Clarke, CJS (1986). Singularities: global and local aspects Topological properties and global structure of spacetime. New York: Plenum Press
- De, UC, and De, BK (2008). On quasi-Einstein manifolds. Commun Korean Math Soc. 23, 413-420.
- De, UC, and Ghosh, GC (2004). On quasi-Einstein manifolds. Period Math Hungar. 48, 223-231.
- De, UC, and Ghosh, GC (2004). On generalized quasi-Einstein manifolds. Kyungpook Math J. 44, 607-615.
- De, UC, Guha, N, and Kamilya, D (1995). On generalized Ricci-recurrent manifolds. Tensor (NS). 56, 312-317.
- De, UC, Jun, JB, and Gazi, AK (2008). Sasakian manifolds with quasi-conformal curvature tensor. Bull Korean Math Soc. 45, 313-319.
- De, UC, and Mallick, S (2014). Spacetimes admitting W2-curvature tensor. Int J Geom Methods Mod Phys. 11, 8.
- De, UC, and Matsuyama, Y (2006). Quasi-conformally flat manifolds satisfying certain conditions on the Ricci tensor. SUT J Math. 42, 295-303.
- De, UC, and Sarkar, A (2012). On the quasi-conformal curvature tensor of a (k, μ)-contact metric manifolds. Math Rep (Bucur). 14, 115-129.
- De, UC, and Velimirović, L (2015). Spacetimes with semisymmetric energy-momentum tensor. Internat J Theoret Phys. 54, 1779-1783.
- Debnath, P, and Konar, A (2011). On super quasi Einstein manifolds. Publ Inst Math. 89, 95-104.
- Geroch, BP (1971). Spacetime structure from a global view point. New York: Academic Press
- Ghosh, GC, De, UC, and Binh, TQ (2006). Certain curvature restrictions on a quasi-Einstein manifold. Publ Math Debrecen. 69, 209-217.
- Guha, S (2003). On a perfect fluid spacetime admitting quasi-conformal curvature tensor. Facta Universitatis. 3, 843-849.
- Hawking, SW, and Ellis, GFR (1973). The large scale structure of space-time. Cambridge Monographs on Mathematical Physics: Cambridge Univ. Press
- Joshi, PS (). Global aspects in gravitation and cosmology. New York: Oxford Science Publications, Oxford University Press, pp. 1993
- Maartens, R (1996). Causal thermodynamics in relativity. Lectures given at the Hanno Rund Workshop on Relativity and Thermodynamics. South Africa, June: Natal University
- Mantica, CA, and Molinari, LG (2012). Weakly Z symmetric manifolds. Acta Math Hunger. 135, 80-96.
- Mantica, CA, and Suh, YJ (2011). Conformally symmetric manifolds and quasi conformally recurrent Riemannian manifolds. Balkan J Geom Appl. 16, 66-77.
- Mantica, CA, and Suh, YJ (2014). Pseudo-Z symmetric space-times. J Math Phys. 55, 12.
- Mocanu, AL (1987). Les varietes a courbure quasi-constant de type Vranceanu. Lucr Conf Nat de Geom Si Top, Tirgoviste.
- Novello, M, and Reboucas, MJ (1978). The stability of a rotating universe. The Astrophysical Journal. 225, 719-724.
- O’neill, B (1983). Semi-Riemannian geometry With applications to relativity. New York: Academic Press Inc
- Özgür, C (2009). On some classes of super quasi-Einstein manifolds. Chaos, Solitons Fractals. 40, 1156-1161.
- Özgür, C, and Sular, S (2008). On N(k)-quasi-Einstein manifolds satisfying certain conditions. Balkan J Geom Appl. 13, 74-79.
- Patterson, EM (1952). Some theorems on Ricci-recurrent spaces. J London Math Soc. 27, 287-295.
- Petrov, AZ (1949). Einstein spaces. Oxford: Pergamon Press
- Schouten, JA (1954). Ricci-calculus. Berlin: Springer
- Shaikh, AA (2009). On pseudo quasi-Einstein manifolds. Period Math Hungar. 59, 119-146.
- Sular, S, and Özgür, C (2012). Characterizations of generalized quasi-Einstein manifolds. An St Univ Ovidius Constanta. 20, 407-416.
- Tamassy, L, and Binh, TQ (1993). On weak symmetries of Einstein and Sasakian manifolds. Tensor (NS). 53, 140-148.
- Vranceanu, Gh (1968). Lecons des Geometrie Differential. Bucharest: Ed.de I’Academie
- Yano, K, and Sawaki, S (1968). Riemannian manifolds admitting a conformal transformation group. J Diff Geom. 2, 161-184.
- Zengin, FÖ (2012). m-Projectively flat spacetimes. Math Reports. 14, 363-370.