Research Note Volume 2 Issue 2
Department of Physics, Kamla Nehru Institute of Physical and Social Sciences, India
Correspondence: Gunraj Prasad, Department of Physics, Kamla Nehru Institute of Physical and Social Sciences, Sultanpur, Uttar Pradesh, India, Tel 9452328706
Received: December 15, 2017 | Published: March 21, 2018
Citation: Prasad G. Non–existence of potential vorticity in a stationary axisymmetric adiabatic fluid configuration. Phys Astron Int J. 2018;2(2):102-103. DOI: 10.15406/paij.2018.02.00069
It is found that the value of relativistic potential vorticity is zero in the case of a stationary axisymmetric adiabatic fluid flows. The fluid’s vorticity flux vector lies in the level surfaces of constant entropy per baryon and thereby leads to conservation of fluid helicity.
Keywords: potential vorticity, fluid’s vorticity, vector, entropy, kelvin’s circulation theorem, fluid helicity, euler’s equation
The conservation of relativistic potential vorticity along adiabatic fluid flow lines in connection with Kelvin’s circulation conservation has been demonstrated by Katz.1 In particular, the stream line invariance of potential vorticity is intimately related to a weak version of Kelvin’s circulation theorem. Bekenstein2 has pointed out that there is an intrinsic relation between potential vorticity and fluid helicity. The purpose of present note is to obtain an explicit expression of fluid vorticity flux3 in a stationary axisymmetric adiabatic fluid flows and use this expression to show that the value of potential vorticity is zero and the fluid helicity is conserved.
We begin with Euler’s equation of motion given by4
Wabub=Ts,aWabub=Ts,a ,(1)
WhereTT andss denote, respectively, the local temperature and the entropy per baryon measured in the fluid’s rest frame.uaua is the 4-velocity of the fluid and obeys the normalization conditionuaua=−1uaua=−1 . The particle vorticity 2-formWabWab is expressible as
Wab=(μub) ;a−(μua) ;b , (2)
Where μ=ρ+pn
denotes the relativistic enthalpy per baryon. Adiabaticity conditionuas,a=0
follows from (1). The proper energy density and pressure are respectively, designated byρ
and p
. The baryon conservation law is given by
(nua) ;a=0
, (3)
Wheren is baryon number density. It follows from (2) that
W[ab;c]=0 , (4)
Where the square bracket around indices denotes skew–symmetrization. Covariant derivative is denoted by semicolon while partial derivative is indicated by comma throughout the present text. It is evident from (1) and (4) that Euler’s equation appears as Maxwell’s like equation. We now assume that the fluid flows are stationary and axisymmetric. We taket andφ to be the time and axial coordinates, respectively, in spherical coordinate system andr , θ are poloidal coordinates. All physical quantities including the metric tensorgab are independent of toroidal coordinatest andφ . In this coordinate system using symmetry assumption we obtain from (1)–(4) the first integrals as follows:
Wφr=An√−guθ , (5)
Wφθ=−An√−gur , (6)
WtrWφr=WtθWφθ=− (say) (7)
Wtr=−An√−guθ , (8)
Wtθ=An√−gur , (9)
Wrθ=An√−g(−ut+uφ)+(Tuθ)s,r . (10)
WhereA is a constant of integration along the fluid flow lines and is called streamline invariant.ˉΩ represents the mechanical rotation of fluid’s vortex lines. The magnetic part ofWab can be defined as
Va=− * Wabub , (11)
WhereVa=2μωa and * Wab=12ηabcdWcd . The vector fieldωa is the fluid’s vorticity and is defined according asωa=12ηabcdub;cud .5 ηabcd is the Levi-Civita alternating tensor. The quantityVa has been referred to as the fluid’s vorticity flux.3 Making use of (5), (6), (8), (9) and (10) in (11), a straightforward calculation yields that
Va=An[(δat+δaφ)+(ut+uφ)ua]+(Tuθ)s,r(δaφut−δatuφ) , (12)
Which exhibits that the spatial variation of the entropy per baryon contributes to the generation of fluid’s vorticity flux in addition to the mechanical rotation of vortex lines. On account of (12) and adibaticity condition, we find that
Vas,a=0 , (13)
Which shows that the vorticity flux vector lies in the level surfaces of constant entropy per baryon. The expression given by (12) is an explicit expression for the fluid’s vorticity flux. The potential vorticity defined by Katz1 ise=μωas,an . Because of (13), it is seen thate=0 . Thus the potential vorticity is zero in a stationary axisymmetric adiabatic fluid flows. The fluid helicity introduced by Bekenstein2 is expressible as
Ha= * Wabμub , (14)
Which in our case takes the formHa=μVa . The fluid helicity is conserved, i.e. Haa=0 because of (13). Further results will be published elsewhere.
None.
Author declares there is no conflict of interest.
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