In this paper, we have deduced an analytic expression for the adiabatic compressibility
for a Chaplygin gas which is a function of the pressure P and temperature T. We have considered the work of Panigrahi (2015) for variable Chaplygin gas, exotic matter used in some cosmological theories whose equation of state is of the form
with
and n is a constant. The expression obtained for
was used for the determination of the value of the thermal capacity at constant pressure
for variable Chaplygin gas. It is predicted in this research the behaviour of the adiabatic compressibility
of Chaplygin gas in the limit of high and low pressure. We have found that the adiabatic compressibility
is function of the pressure and
when
and
if
as in the ideal gas and
is always positive with
n<0.
Adiabatic Compressibility, Chaplygin Gas, Cosmological Theories, Equation of State, Exotic Matter
[1]
Sushkov, S. (2005). Wormholes supported by a phantom energy. Phys. Rev, D71, 043520.
[2]
Lobo, F.S.N. (2005). Stability of phantom wormholes. Phys. Rev, D71, 124022.
[3]
Lobo, F.S.N. (2006). Stable dark energy stars. Class. Quant.Grav, 23, 1525-1541.
[4]
Fabris, J.C., Goncalves S.V.B. and de Souza, P.E. (2002). Gen. Relativ. Grav. 34, 53.
[5]
Lima, J.A.S., Cunha, J.V. and Alcaniz, J.S. (2008). A simplified approach for Chaplygin-type cosmologies.Astropart.Phys.30, 196-199.
[6]
Bento, M.C., Bertolami, O. and Sen, A.A. (2002). Phys.Rev. D66, 043507.
[7]
Panigrahi, D. and Chaterjee, S. (2011). JCAP 10 002.
[8]
Santos, F.C., Bedran, M.L. and Soares, V. (2006). Phys.Lett. B636, 86.
[9]
Guo, Z.K. and Zhang, Y.Z. (2007). Phys. Lett. B645, 326.
[10]
Myung, Y.S. (2011). Thermodynamics of Chaplygin gas.Astrophys.Space Sci.335,561-564.
[11]
Panigrahi, D. (2015). Thermodynamicalbehaviour of the variable Chaplygin gas.Int.J.Mod.Phys.D24, 1550030.
[12]
Leff, H.S.(2002). Teaching the photon gas in introductory physics. Am. J. Phys, 70, 792-797.
[13]
Wang, S., Wu, S-Q., Xie, F. and Dan, L. (2006). Chin. Phys. Lett. 23, 1096.
[14]
Sekiwa, Y. (2006). Phys. Rev. D73, 084009.
[15]
Larrañaga, E.A. (2007). http://arxiv.org/abs/0711.0012
[16]
Dolan, B.P. (2011). Compressibility of rotating black holes.Phys.Rev, D84,127503.
[17]
Lee, H. (2001). Carnot cycle for photon gas? Am.J.Phys, 69, 874-878.
[18]
Malaver, M. (2015). Carnot engine model in a Chaplygin gas.Research Journal ofModeling and Simulation, 2(2), 42-47.
[19]
Dickerson, R.(1969). MolecularThermodynamics, W.A.Benjamin, Inc, Menlo Park,California, ISBN: 0-8053-2363-5.
[20]
Nash, L.(1970). Elements of Classical and Statistical Thermodynamics, Addison-Wesley Publishing Company, Inc, MenloPark, California.
[21]
Zemansky, M.W. andDittman,R.H. (1985). Termodinámica, McGraw-Hill Interamericana, Sexta Edición,ISBN: 0-07-72808-9.