Deviations from the von Laue Condition: Implications for the On-Shell Lagrangian of Particles and Fluids

• DOI: 10.48550/arxiv.2502.10427
• Publication Date: 2025-01-01
• Authors: Pinto, S. R.; Avelino, P. P.
• Keywords: High Energy Physics - Phenomenology; Cosmology and Nongalactic Astrophysics (astro-ph.CO); High Energy Physics - Phenomenology (hep-ph); FOS: Physical sciences; General Relativity and Quantum Cosmology (gr-qc); General Relativity and Quantum Cosmology; Astrophysics - Cosmology and Nongalactic Astrophysics

According to the von Laue condition, the volume integral of the proper pressure inside isolated particles with a fixed structure and finite mass vanishes in the Minkowski limit of general relativity. In this work, we consider a simple illustrative example: non-standard static global monopoles with finite energy, for which the von Laue condition is satisfied when the proper pressure is integrated over the whole space. We demonstrate, however, that the absolute value of this integral, when calculated up to a finite distance from the center of the global monopole, generally deviates from zero, and that this deviation is bounded by the energy located outside the specified volume (under the assumption of the dominant energy condition). Furthermore, we find that the maximum deviation from unity of the ratio between the volume averages of the on-shell Lagrangian and the trace of the energy-momentum tensor cannot exceed three times the outer energy fraction. Additionally, we show that, as long as the dominant energy condition holds, these constraints generally apply to real particles with fixed structure and finite mass. We discuss the implications of this result in the context of stable atomic nuclei. Specifically, we argue that, except in extremely dense environments with energy densities comparable to that of an atomic nucleus (e.g., inside neutron stars), the volume average of the aforementioned ratio for atomic nuclei should remain extremely close to unity. Finally, we discuss the implications of our findings for the form of the on-shell Lagrangian of real fluids. This is often a crucial element for accurately describing fluid dynamics in the presence of non-minimal couplings to other matter fields or gravity.<br/>9 pages, 7 figures<br/>