Scalar Pre-potentials for Spinor and Tensor Fields on Spacetime

نویسندگان

چکیده

Abstract We review a technique for solving class of classical linear partial diferential systems relevance to physics in Minkowski spacetime. All the equations are amenable analysis terms complex solutions kernel scalar Laplacian and complexifed Hertz potential. The complexifcation prescription ensures existence regular physical with chirality propagating, non-singular, pulse-like characteristics that bounded all three spatial dimensions. is applied source-free Maxwell, Bopp-Landé-Podolsky linearised Einstein feld systems, particular used constructing models describing single-cycle laser pulses mechanism discussed initiating astrophysical jets. Our article concludes brief introduction spacetime Cliford algebra ideals we use represent spinor felds. employ these demonstrate how same tensor felds enables one construct new chiral, massless Dirac equation

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Note on the energy-momentum tensor for general mixed tensor-spinor fields

This note provides an explicit proof of the equivalence of the Belinfante’s energy-momentum tensor and the metric energy-momentum tensor for general mixed tensor-spinor fields.

متن کامل

Nonlinear Spinor and Scalar Fields in General Relativity

We consider a system of nonlinear spinor and scalar fields with minimal coupling in general relativity. The nonlinearity in the spinor field Lagrangian is given by an arbitrary function of the invariants generated from the bilinear spinor forms S = ψ̄ψ and P = iψ̄γ5ψ; the scalar Lagrangian is chosen as an arbitrary function of the scalar invariant Υ = φ,αφ ,α, that becomes linear at Υ → 0. The sp...

متن کامل

Scalar and spinor fields in signature-changing spacetimes.

The propagation of scalar and spinor fields in a spacetime whose metric changes signature is analyzed. Recent work of Dray et al. on particle production from signature change for a (massless) scalar field is reviewed, and an attempt is made to extend their analysis to the case of a (massless) spin-half field. In contrast to their results for a scalar field, it is shown here—for SL(2, C) spinors...

متن کامل

Adiabatic Geometrical Phase for Scalar Fields in a Curved Spacetime

A convenient framework is developed to generalize Berry’s investigation of the adiabatic geometrical phase for a classical relativistic charged scalar field in a curved background spacetime which is minimally coupled to electromagnetism and an arbitrary (non-electromagnetic) scalar potential. The general formalism which is applicable for any scalar field equation which involves time derivatives...

متن کامل

Quantum interest for scalar fields in Minkowski spacetime

The quantum interest conjecture of Ford and Roman states that any negative energy flux in a free quantum field must be preceded or followed by a positive flux of greater magnitude, and the surplus of positive energy grows the further the positive and negative fluxes are apart. In addition, the maximum possible separation between the positive and negative energy decreases the larger the amount o...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Journal of physics

سال: 2022

ISSN: ['0022-3700', '1747-3721', '0368-3508', '1747-3713']

DOI: https://doi.org/10.1088/1742-6596/2191/1/012020