Relativistic system (mathematics)

In mathematics, a non-autonomous system of ordinary differential equations is defined to be a dynamic equation on a smooth fiber bundle $Q\to \mathbb R$ over $\mathbb R$ . For instance, this is the case of non-relativistic non-autonomous mechanics, but not relativistic mechanics. To describe relativistic mechanics, one should consider a system of ordinary differential equations on a smooth manifold $Q$ whose fibration over $\mathbb R$ is not fixed. Such a system admits transformations of a coordinate $t$ on $\mathbb R$ depending on other coordinates on $Q$ . Therefore, it is called the relativistic system. In particular, Special Relativity on the Minkowski space $Q= \mathbb R^4$ is of this type.

Since a configuration space $Q$ of a relativistic system has no preferable fibration over $\mathbb R$ , a velocity space of relativistic system is a first order jet manifold $J^1_1Q$ of one-dimensional submanifolds of $Q$ . The notion of jets of submanifolds generalizes that of jets of sections of fiber bundles which are utilized in covariant classical field theory and non-autonomous mechanics. A first order jet bundle $J^1_1Q\to Q$ is projective and, following the terminology of Special Relativity, one can think of its fibers as being spaces of the absolute velocities of a relativistic system. Given coordinates $(q^0, q^i)$ on $Q$ , a first order jet manifold $J^1_1Q$ is provided with the adapted coordinates $(q^0,q^i,q^i_0)$ possessing transition functions

q'^0=q'^0(q^0,q^k), \quad q'^i=q'^i(q^0,q^k), \quad {q'}^i_0 = \left(\frac{\partial q'^i}{\partial q^j} q^j_0 + \frac{\partial q'^i}{\partial q^0} \right) \left(\frac{\partial q'^0}{\partial q^j} q^j_0 + \frac{\partial q'^0}{\partial q^0} \right)^{-1}.

The relativistic velocities of a relativistic system are represented by elements of a fibre bundle $\mathbb R\times TQ$ , coordinated by $(\tau,q^\lambda,a^\lambda_\tau)$ , where $TQ$ is the tangent bundle of $Q$ . Then a generic equation of motion of a relativistic system in terms of relativistic velocities reads

\left(\frac{\partial_\lambda G_{\mu\alpha_2\ldots\alpha_{2N}}}{2N}- \partial_\mu G_{\lambda\alpha_2\ldots\alpha_{2N}}\right) q^\mu_\tau q^{\alpha_2}_\tau\cdots q^{\alpha_{2N}}_\tau - (2N-1)G_{\lambda\mu\alpha_3\ldots\alpha_{2N}}q^\mu_{\tau\tau} q^{\alpha_3}_\tau\cdots q^{\alpha_{2N}}_\tau + F_{\lambda\mu}q^\mu_\tau =0,

G_{\alpha_1\ldots\alpha_{2N}}q^{\alpha_1}_\tau\cdots q^{\alpha_{2N}}_\tau=1.

For instance, if $Q$ is the Minkowski space with a Minkowski metric $G_{\mu\nu}$ , this is an equation of a relativistic charge in the presence of an electromagnetic field.

References

Krasil'shchik, I. S., Vinogradov, A. M., [et al.], "Symmetries and conservation laws for differential equations of mathematical physics", Amer. Math. Soc., Providence, RI, 1999, ISBN 0-8218-0958-X.
Giachetta, G., Mangiarotti, L., Sardanashvily, G., Geometric Formulation of Classical and Quantum Mechanics (World Scientific, 2010) ISBN 981-4313-72-6 (arXiv: 1005.1212).

Relativistic system (mathematics)

References

See also