Torsion: what it is and how does it work
Paweł Laskoś-Grabowski
Institute for Theoretical Physics, University of Wrocław
January 10, 2009
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 1 / 25
Introduction Conventions
Outline
1
Introduction
Conventions
Einstein Cartan theory
2
Mathisson Papapetrou equation
Free spinning particle
Particle in gravitational field
3
Finish
Motivations and conclusions
Bibliography
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 2 / 25
Introduction Conventions
Basic symbols & conventions
D = 4
c = = 1
= diag(-, +, +, +)
Greek indices correspond to the curved space. Latin indices
correspond to the tangent space.
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 3 / 25
Introduction Einstein Cartan theory
Outline
1
Introduction
Conventions
Einstein Cartan theory
2
Mathisson Papapetrou equation
Free spinning particle
Particle in gravitational field
3
Finish
Motivations and conclusions
Bibliography
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 4 / 25
Introduction Einstein Cartan theory
Poincar group
Initially devised to be the symmetry group of Maxwell equations
Consists of (local) translations, rotations and boosts
Algebra consists of 10 generators: momenta and angular momenta
Commutation relations:
[P, P] = 0
[J, P] = i(P - P)
[J, J] = i(J - J - J + J)
We now choose it to be group of fundamental symmetries of our
theory
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 5 / 25
Introduction Einstein Cartan theory
Differential forms
Coordinate-independent approach
ą a" ąi1i2...ik dxi1 '" dxi2 '" . . . '" dxik
Wedge product: ą '" is a form of greater rank
Exterior derivative dą:
"ąi1i2...ik
dą = dxi1 '" dxi2 '" . . . '" dxik '" dxj
"xj
j
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 6 / 25
Introduction Einstein Cartan theory
Einstein Cartan theory
Gauge fields for Poincar group
a
Translations Pa field of frames ea a" e dx
ab
Lorentz rotations &!ab = -&!ba field of connection ab a" dx
Transformations under Lorentz group element
= T - (d)T
e = e
Transformations under translation a
=
e = e + d +
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 7 / 25
Introduction Einstein Cartan theory
Curvature and torsion
Two important two-forms
Rab = dab + a '" cb
c
a
T = dea + a '" eb
b
Bianchi identity (curvature is covariant constant)
dR = dd + d( '" ) = d '" - '" d
= d '" + '" '" - '" d - '" '"
= (d + '" ) '" - '" (d + '" ) = R '" - '" R
Similar identity for torsion
dT = dde + d( '" e) = d '" e - '" de
= d '" e + '" '" e - '" de - '" '" e
= (d + '" ) '" e - '" (de + '" e) = R '" e - '" T
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 8 / 25
Introduction Einstein Cartan theory
Relation to classical general relativity
a b
e is invertible g = abee
May be proven that
1 a a a
Ra - bR + b = T
b 2 b
a a d a d a
Tbc = Sbc + Sdbc - Sdcb
D-2 D-2
Classical GR assumes also T = 0 and e = const. Everything, incl. R
may then be expressed in terms of g.
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 9 / 25
Mathisson Papapetrou equation Free spinning particle
Outline
1
Introduction
Conventions
Einstein Cartan theory
2
Mathisson Papapetrou equation
Free spinning particle
Particle in gravitational field
3
Finish
Motivations and conclusions
Bibliography
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 10 / 25
Mathisson Papapetrou equation Free spinning particle
Representation
Particles represented as elements of connected Poincar group
ę!
P+ = R4 Lę! = {(z, )}
+
z coordinates of particle location
relates to momentum and spin:
pa = ma0, m > 0
1
Sabab = 12-1 a" -iS
2
a b a b
where (ab)cd = -i(c d - dc ), = const
1
It follows that SabSab = 2, paSab = 0
2
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 11 / 25
Mathisson Papapetrou equation Free spinning particle
Free lagrangian
1
Classical spinning particle: L0 = m 2 + i Tr(3s-1a)
2
Ł
Relativistic analogue: Lp = paża + i Tr(12-1)
2
Variation w.r.t. z obviously Wa = 0
General variation of is of such form: = i
Then follows -1 = -i-1 because
0 = (-1) = -1 + -1 = i -1 + -1
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 12 / 25
Mathisson Papapetrou equation Free spinning particle
Free lagrangian (cont.)
Variation w.r.t.
If kab = żapb = (zapb) , then
(paża) = mżaa0 = mi( )abbża
0
= -i( )bakab = -i Tr( k)
The other term yields
Ł Ł
i (Tr(12-1)) = i Tr(12 -i-1( ))
2 2
+ i Tr(12-1i( ) )
2
Ł
+ i Tr(12-1i( ))
2
i
= Tr(i12-1( ) )
2
S
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 13 / 25
Mathisson Papapetrou equation Free spinning particle
Free lagrangian (cont.)
Angular momentum conservation
i
Full variation now reads Lp = -i Tr(k ) + Tr(S( ) )
2
1
Integrating by parts gives Lp = -i Tr((zapb + Sab) ( ))
2
Conserved charge total angular momentum:
Mab = zapb - zbpa + Sab
If we expand @ = 0, multiply by pa and recall that pa`ab = 0, we ll
obtain p ż
"
Furthermore, then pa = mża/ -ż2 and `ab = 0
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 14 / 25
Mathisson Papapetrou equation Particle in gravitational field
Outline
1
Introduction
Conventions
Einstein Cartan theory
2
Mathisson Papapetrou equation
Free spinning particle
Particle in gravitational field
3
Finish
Motivations and conclusions
Bibliography
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 15 / 25
Mathisson Papapetrou equation Particle in gravitational field
Lagrangian with fields
Analogous design of lagrangian
a
L = paeż + i Tr(12-1D ) + field part
2
ab
Ł
Covariant derivative (D )a = a + ż cb
b b
Varying w.r.t. is formally identical
i
L = -i Tr(J ) + Tr(SD ( ))
2
a
where Jab = eżpb
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 16 / 25
Mathisson Papapetrou equation Particle in gravitational field
Lagrangian with fields (cont.)
Spin precession equation
Carrying on. . .
i
L = -i Tr(J ) + Tr(S( ) + S[ż, ])
2
i
a" -i Tr(J ) + Tr(-` + Sż - żS )
2
1
= -i Tr((J + D S) )
2
EOM: Jab - Jba + (D S)ab = 0
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 17 / 25
Mathisson Papapetrou equation Particle in gravitational field
Lagrangian with fields (cont.)
Varying w.r.t. z
This will hurt only for a while. . .
a a
L = paeż + pażz"e + i Tr(12-1(ż + żz"))
2
1
a a
= paeż + pażz"e + Tr(S(ż + żz"))
2
1
a a
a" -(pae) z + pażz"e + Tr(-` - S + Sż")z
Ł
2
If Jab = Jab - Jba then 0 = J + D S = J + ` + [ż, S], so we expand
` = -J - [ż, S] into the following
L 1
a a
= -(pae) + paż"e + Tr(J + [ż, S] - S + Sż")
Ł
z 2
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 18 / 25
Mathisson Papapetrou equation Particle in gravitational field
Lagrangian with fields (cont.)
Varying w.r.t. z (cont.)
We will now apply three simplifications at once:
" dz
= = "ż
Ł
d
"z
Tr([ż, S]) = Tr(żS - Sż) = Tr(żS[, ])
ba ab ab
Tr(J) = (Jab - Jba) = -2Jab = -2ea żpb
L
a a ab
= -(pae) + paż"e - ea żpb
z
1
+ Tr(żS[, ] - żS" + żS")
2
. . . and " - " + [, ] = R!
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 19 / 25
Mathisson Papapetrou equation Particle in gravitational field
And we re done!
Now we expand the first term
a a a a a
(pae) = Wae + pa = (D pa - żab pb)e + paż"e
After insertion we see
L 1
a
= -eD pa + ż Tr(SR)
z 2
a a a ab
+ żab pbe - paż"e + paż"e - ea żpb
a a a b a b
paż ("e - "e + be - be)
a
T
Mathisson Papapetrou equation (with torsion)
1
a a
(D pa)e = pażT + ż Tr SR
2
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 20 / 25
Finish Motivations and conclusions
Outline
1
Introduction
Conventions
Einstein Cartan theory
2
Mathisson Papapetrou equation
Free spinning particle
Particle in gravitational field
3
Finish
Motivations and conclusions
Bibliography
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 21 / 25
Finish Motivations and conclusions
What s all this for?!
E C theory allows us to consider spinning particles
No inherent reason for T = 0
What is torsion itself, anyway?
Simpliest physical realisation of translation movement of a test
particle by a fixed amount of affine parameter
MP equation leads to EOMs for particles in contorted spacetime
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 22 / 25
Finish Motivations and conclusions
What s all this for?!
Curvature
Vector is rotated, when transported along a closed path
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 22 / 25
Finish Motivations and conclusions
What s all this for?!
Torsion
Closed paths don t close , i.e. translation addition doesn t commute
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 22 / 25
Finish Motivations and conclusions
What s all this for?!
E C theory allows us to consider spinning particles
No inherent reason for T = 0
What is torsion itself, anyway?
Simpliest physical realisation of translation movement of a test
particle by a fixed amount of affine parameter
MP equation leads to EOMs for particles in contorted spacetime
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 22 / 25
Finish Bibliography
Outline
1
Introduction
Conventions
Einstein Cartan theory
2
Mathisson Papapetrou equation
Free spinning particle
Particle in gravitational field
3
Finish
Motivations and conclusions
Bibliography
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 23 / 25
Finish Bibliography
Selected references & further reading
Meissner KA, Klasyczna teoria pola, PWN, Warsaw 2002
Balachandran AP, Marmo G, Skagerstam B-S, Stern A, Gauge
Symmetries and Fibre Bundles. Applications to Particle Dynamics,
Springer 1983
Nakahara M, Geometry, Topology and Physics, IOP 2003
Mathisson M, Neue Mechanik materieller Systeme, Acta Phys Polon 6
(1937) 163 200
Freidel L, Kowalski-Glikman J, Starodubtsev A, Particles as Wilson
lines of gravitational field, 2008,gr-qc/0607014v2
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 24 / 25
Myron Mathisson
Warsaw 1897 Cambridge 1940
Paweł Laskoś-Grabowski (IFT UWr) Torsion January 10, 2009 25 / 25
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