A New Model for Gravitational Waves

QUEST Center event
No
Speaker
Yaakov Friedman, Jerusalem College of Technology (Lev)
Date
08/07/2025 - 15:00 - 13:30Add to Calendar 2025-07-08 13:30:00 2025-07-08 15:00:00 A New Model for Gravitational Waves Gravitational waves are among the most striking predictions of General Relativity (GR), yet alternative formulations may offer fresh insights into their nature. In this talk, I present a novel approach to relativistic gravity called Extended Relativity, which, like GR, treats gravity as a manifestation of spacetime geometryCentral to this model is a new metric for a single point mass, which aligns with all classical tests of GR. Building on this, a superposition principle—reminiscent of the linearity in electromagnetism—allows us to construct the gravitational field for multiple sources.Notably, when a mass accelerates, it produces a "far-field" component in its gravitational field, akin to how accelerating charges emit electromagnetic radiation. In systems like binary stars, this far-field behaves similarly to the quadrupole radiation predicted by GR, leading to wave-like effects that mirror gravitational waves.This model not only reproduces the essential predictions of GR but also provides a framework for describing relativistic corrections in galactic dynamics.***NOTE UNUSUAL DAY - TUESDAY*** Physics Building 202 Seminar Room 303 המחלקה לפיזיקה physics.dept@mail.biu.ac.il Asia/Jerusalem public
Place
Physics Building 202 Seminar Room 303
Abstract

Gravitational waves are among the most striking predictions of General Relativity (GR), yet alternative formulations may offer fresh insights into their nature. In this talk, I present a novel approach to relativistic gravity called Extended Relativity, which, like GR, treats gravity as a manifestation of spacetime geometry

Central to this model is a new metric for a single point mass, which aligns with all classical tests of GR. Building on this, a superposition principle—reminiscent of the linearity in electromagnetism—allows us to construct the gravitational field for multiple sources.

Notably, when a mass accelerates, it produces a "far-field" component in its gravitational field, akin to how accelerating charges emit electromagnetic radiation. In systems like binary stars, this far-field behaves similarly to the quadrupole radiation predicted by GR, leading to wave-like effects that mirror gravitational waves.

This model not only reproduces the essential predictions of GR but also provides a framework for describing relativistic corrections in galactic dynamics.

***NOTE UNUSUAL DAY - TUESDAY***

תאריך עדכון אחרון : 12/05/2025