arXiv subjects

Guido Magnano

Publications and source records attributed to Guido Magnano.

11 recordsLinked to original sources

arXiv2025

Einstein's elevator and the principle of equivalence

We outline here the design, execution, and educational outcomes of an intervention inspired by Einstein's elevator thought experiment, intended to introduce secondary school students to the principle of equivalence, which is at the basis of the theory of General Relativity. We build an experimental version of Einstein's elevator, which simulated the effects of free-fall in an accelerated reference frame: a detailed description of the experimental apparatus and its construction is provided, highlighting the challenges and innovations in creating a simple yet functional setup using everyday materials.

physics.ed-ph↗

arXiv2023

On the "Legendre scalarization" of nonlinear gravity theories

We discuss the proposal of a new method to transform a f(R) metric gravity theory into a general relativistic theory including an auxiliary scalar field, recently introduced by S. Cotsakis et al. We argue that (i) the fact that the fourth order equations of f(R) metric gravity can be recast (via a Legendre transformation) into Einstein equations without any conformal rescaling has been thoroughly clarified in the previous literature, and (ii) the newly proposed method produces a set of equations that are not equivalent to the original theory. In the conclusion, a comment is added on another aspect of the Legendre transformation which seems to be generally overlooked.

gr-qc↗

arXiv2021

On the Generalised Equipartition Law

We observe that the so-called Generalised Equipartition Law for hamiltonian systems is actually valid only under specific hypotheses -- unfortunately omitted in some textbooks -- which limit its applicability when dealing with nonlinear systems. We introduce a new coordinate-independent generalisation which overcomes this problem, and moreover can be applied to a larger set of functions. A simple example of application is discussed.

math-ph↗

arXiv2020

New Separation of Variables for the Classical XXX and XXZ Heisenberg Spin Chains

We propose a non-standard separation of variables for the classical integrable XXX and XXZ spin chains with degenerate twist matrix. We show that for the case of such twist matrices one can interchange the role of classical separating functions $A(u)$ and $B(u)$ and construct a new full set of separated variables, satisfying simpler equation of separation and simpler Abel equations in comparison with the standard separated variables of Sklyanin. We show that for certain cases of the twist matrices the constructed separated variables can be directly identified with action-angle coordinates.

math-ph↗

arXiv2019

Test-field limit of metric nonlinear gravity theories

In the framework of alternative metric gravity theories, it has been shown by several authors that a generic Lagrangian depending on the Riemann tensor describes a theory with 8 degrees of freedom (which reduce to 3 for f(R) Lagrangians depending only on the curvature scalar). This result is often related to a reformulation of the fourth-order equations for the metric into a set of second-order equations for a multiplet of fields, including a massive scalar field and a massive spin-2 field. In this article we investigate an issue which does not seem to have been addressed so far: in ordinary general-relativistic field theories, all fundamental fields (i.e. fields with definite spin and mass) reduce to test fields in some appropriate limit of the model, where they cease to act as sources for the metric curvature. In this limit, each of the fundamental fields can be excited from its ground state independently from the others. The question is: does higher-derivative gravity admit a test-field limit for its fundamental fields? It is easy to show that for a f(R) theory the test-field limit does exist; then, we consider the case of Lagrangians quadratically depending on the full Ricci tensor. We show that the constraint binding together the scalar field and the massive spin-2 field does not disappear in the limit where they should be expected to act as test fields, except for a particular choice of the Lagrangian, which cause the scalar field to disappear (reducing to 7 DOF). We finally consider the addition of an arbitrary function of the quadratic invariant of the Weyl tensor and show that the resulting model still lacks a proper test-field limit. We argue that the lack of a test-field limit for the fundamental fields may constitute a serious drawback of the full 8 DOF higher-order gravity models, which is not encountered in the restricted 7 DOF or 3 DOF cases.

gr-qc↗

arXiv2016

Nonlinear Gravitational Lagrangians revisited

The Legendre transformation method, applied in 1987 to deal with purely metric gravitational Lagrangians with nonlinear dependence on the Ricci tensor, is extended to metric-affine models and is shown to provide a concise and insightful comparison of the dynamical content of the two variational frameworks.

gr-qc↗

arXiv2005

A trihamiltonian extension of the Toda lattice

A new Poisson structure on a subspace of the Kupershmidt algebra is defined. This Poisson structure, together with other two already known, allows to construct a trihamiltonian recurrence for an extension of the periodic Toda lattice with $n$ particles. Some explicit examples of the construction and of the first integrals found in this way are given.

nlin.SI↗

arXiv2002

Symmetry properties of the metric energy-momentum tensor in classical field theories and gravity

We derive a generic identity which holds for the metric (i.e. variational) energy-momentum tensor under any field transformation in any generally covariant classical Lagrangian field theory. The identity determines the conditions under which a symmetry of the Lagrangian is also a symmetry of the energy-momentum tensor. It turns out that the stress tensor acquires the symmetry if the Lagrangian has the symmetry in a generic curved spacetime. In this sense a field theory in flat spacetime is not self-contained. When the identity is applied to the gauge invariant spin-two field in Minkowski space, we obtain an alternative and direct derivation of a known no-go theorem: a linear gauge invariant spin-2 field, which is dynamically equivalent to linearized General Relativity, cannot have a gauge invariant metric energy-momentum tensor. This implies that attempts to define the notion of gravitational energy density in terms of the metric energy--momentum tensor in a field-theoretical formulation of gravity must fail.

gr-qc↗

arXiv1998

Can the local stress-energy conservation laws be derived solely from field equations?

According to a recent suggestion [1], the energy--momentum tensor for gravitating fields can be computed through a suitable rearrangement of the matter field equations, without relying on the variational definition. We show that the property observed by Accioly et al. in [1] is the consequence of a general identity, which follows from the covariance of the matter Lagrangian in much the same way as (generalized) Bianchi identities follow from the covariance of the purely gravitational Lagrangian. However, we also show that only in particular cases can this identity be used to obtain the actual form of the stress-energy tensor, while in general the method leads to ambiguities and possibly to wrong results. Moreover, in nontrivial cases the computations turn out to be more difficult than the standard variational technique.

gr-qc↗

arXiv1995

Are there metric theories of gravity other than General Relativity?

Current generalizations of the classical Einstein-Hilbert Lagrangian formulation of General Relativity are reviewed. Some alternative variational principles are known to reproduce Einstein's gravitational equations, and should therefore be regarded as equivalent descriptions of the same physical model, while other variational principles ("Scalar-tensor theories" and "Higher-derivative theories") are commonly presented as truly alternative physical theories. Such theories, however, are also known to admit a reformulation which is formally identical to General Relativity (with auxiliary fields). The physical significance of this change of variables has been questioned by several authors in recent years. Here, we investigate to which extent purely affine, metric-affine, scalar-tensor and purely metric theories can be regarded as physically equivalent to GR; we show that in general this depends on which metric tensorfield is assumed to represent the true physical space-time geometry. For purely metric theories where the Lagrangian is a nonlinear function f(R) of the curvature scalar, we present an argument based on the definition of the physical energy, which leads one to regard the rescaled metric (Einstein frame) as the true physical one. As a direct consequence, the physical content of such "alternative" models is reset to coincide with General Relativity, and the "Nonlinear Gravity Theories" become nothing but exotic reformulations of General Relativity in terms of unphysical variables.

gr-qc↗

arXiv1993

On Physical Equivalence between Nonlinear Gravity Theories

We argue that in a nonlinear gravity theory, which according to well-known results is dynamically equivalent to a self-gravitating scalar field in General Relativity, the true physical variables are exactly those which describe the equivalent general-relativistic model (these variables are known as Einstein frame). Whenever such variables cannot be defined, there are strong indications that the original theory is unphysical. We explicitly show how to map, in the presence of matter, the Jordan frame to the Einstein one and backwards. We study energetics for asymptotically flat solutions. This is based on the second-order dynamics obtained, without changing the metric, by the use of a Helmholtz Lagrangian. We prove for a large class of these Lagrangians that the ADM energy is positive for solutions close to flat space. The proof of this Positive Energy Theorem relies on the existence of the Einstein frame, since in the (Helmholtz--)Jordan frame the Dominant Energy Condition does not hold and the field variables are unrelated to the total energy of the system.

gr-qc↗