# Light-Cones, Almost Light-Cones and Almost-Complex Light-Cones

## TL;DR

This paper explores various null geodesic congruences in Minkowski and asymptotically flat spacetimes, revealing their geometric properties and how they relate to gravitational radiation analysis, offering new coordinate approaches that connect to classical mechanics.

## Contribution

It introduces and characterizes Light-Cones, Almost-Complex Light-Cones, and Almost Light-Cones, highlighting their geometric similarities and potential applications in gravitational radiation studies.

## Key findings

- Null geodesic congruences are shear-free or asymptotically shear-free.
- These congruences can be labeled by points in real or complex 4D manifolds.
- Using Almost Light-Cones simplifies relations in Einstein-Maxwell equations.

## Abstract

We point out an unusual relationship among a variety of null geodesic congruences; (a) the generators of ordinary light-cones and (b) certain (related) shear-free but twisting congruences in Minkowski Space-time as well as (c) asymptotically shear-free null geodesic congruences that exist in the neighborhood of Penrose's Scri in Einstein or Einstein-Maxwell asymptotically flat-space-times. We refer to these geodesic congruences respectively as: Lignt-Cones (LCs), as Almost-Complex- Light-Cones, (ACLCs), [though they are real they resemble complex light-cones in complex Minkowski space] and finally to a family of congruences in asymptotically flat-spaces as `Almost Light-Cones', (ALC). The two essential points of resemblance among the three families are: (1) they are all either shear-free or asymptotically shear-free and (2) in each family the individual members of the family can be labeled by the points in a real or complex four-dimensional manifold. As an example, the Minkowski space LCs are labeled by the (real) coordinate value of their apex. In the case of (ACLCs) (complex coordinate values), the congruences will have non-vanishing twist whose magnitude is determined by the imaginary part of the complex coordinate values. In studies of gravitational radiation, Bondi-type of null surfaces and their associated Bondi coordinates have been almost exclusively used for calculations. Some surprising relations arise if, instead of the Bondi coordinates, one uses ALCs and their associated coordinate systems in the analysis of the Einstein-Maxwell equations near Scri. More explicitly and surprisingly, the asymptotic Bianchi Identities expressed in the coordinates of the ALCs, turn directly into many of the standard definitions and relations of classical mechanics.