No (Lorentz) Invariant tensor of rank 3?

maverick280857
Messages
1,774
Reaction score
5
Hi everyone,

(This isn't a homework problem). How does one show that there is no Lorentz invariant tensor of rank 3 and the only Lorentz invariant tensor of rank 4 is the 4D Levi Civita tensor?

Thanks in advance.
 
Physics news on Phys.org
Let \epsilon^{\mu\nu\rho\sigma}=-1,+1 when the indices are in "even" and "odd" order, respectively. Consider the transformation \epsilon^{\mu\nu\rho\sigma}\Lambda^{\alpha}_{\mu}\Lambda^{\beta}_{\nu}\Lambda^{\gamma}_{\rho}\Lambda^{\delta}_{\sigma}. Writing this out a bit you can show this is the same as writing - or + det|\Lambda|, which gives -1 or +1 when the order of indices on epsilon is "even" or "odd", respectively. This verifies that the transformed epsilon is the same.

Consider instead a rank-3 tensor T^{\mu\nu\rho}\Lambda^{\alpha}_{\mu}\Lambda^{\beta}_{\nu}\Lambda^{\gamma}_{\rho}. No matter what the symmetrization is on the tensor T, you can see that the resulting tensor depends on the transformation parameters in the Lambdas, because only in the case of the rank-d anti-symmetric tensor in d-dimensions can you get that special "det" result...and that, in turn, only worked since the transformations were "special" in the sense of having unit determinant. Such tensors are in fact always proportional to the basic "invariant volume element" you use, e.g., in an integral.
 
Okay, but how do you argue that the Levi Civita is the only rank 4-invariant tensor in 4D?
 
In Philippe G. Ciarlet's book 'An introduction to differential geometry', He gives the integrability conditions of the differential equations like this: $$ \partial_{i} F_{lj}=L^p_{ij} F_{lp},\,\,\,F_{ij}(x_0)=F^0_{ij}. $$ The integrability conditions for the existence of a global solution ##F_{lj}## is: $$ R^i_{jkl}\equiv\partial_k L^i_{jl}-\partial_l L^i_{jk}+L^h_{jl} L^i_{hk}-L^h_{jk} L^i_{hl}=0 $$ Then from the equation: $$\nabla_b e_a= \Gamma^c_{ab} e_c$$ Using cartesian basis ## e_I...
Abstract The gravitational-wave signal GW250114 was observed by the two LIGO detectors with a network matched-filter signal-to-noise ratio of 80. The signal was emitted by the coalescence of two black holes with near-equal masses ## m_1=33.6_{-0.8}^{+1.2} M_{⊙} ## and ## m_2=32.2_{-1. 3}^{+0.8} M_{⊙}##, and small spins ##\chi_{1,2}\leq 0.26 ## (90% credibility) and negligible eccentricity ##e⁢\leq 0.03.## Postmerger data excluding the peak region are consistent with the dominant quadrupolar...
Insights auto threads is broken atm, so I'm manually creating these for new Insight articles. The Relativator was sold by (as printed) Atomic Laboratories, Inc. 3086 Claremont Ave, Berkeley 5, California , which seems to be a division of Cenco Instruments (Central Scientific Company)... Source: https://www.physicsforums.com/insights/relativator-circular-slide-rule-simulated-with-desmos/ by @robphy
Back
Top