hvirgen
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I know light is affected by gravity, but does light have its own gravitational pull? Does light attract other light?
In general relativity, light does possess a gravitational influence, affecting other light beams through its energy density and momentum flow. While light is massless, it can still create a gravitational field, leading to deflection in a gravitational field, such as that produced by a star. The concept of a uniform gravitational field, which has zero spacetime curvature, is clarified through Einstein's equivalence principle, indicating that gravitational effects can exist without tidal forces. This discussion emphasizes the nuanced understanding of light's interaction with gravity and the importance of referencing established physics literature for deeper insights.
PREREQUISITESPhysicists, students of general relativity, and anyone interested in the gravitational interactions of light and their implications in modern physics.
That is not quite true. Although the spacetime is curved around, say, a star it is not curved spacetime that is the cause. For example; a beam of light is deflected by the sun due to the gravitational attraction on the light. The amount of delfection is determined by that acceleration and the amount of spatial contraction caused by the mass of the sun.spidey said:Light has no gravitational field around it..light is bent because space-time is curved as per GR...
Its pretty simple. Eintein never said that gravity was a curvature in spacetime. Actually he stated quite clearly that he disagreed with such an interpretation. The assumption that he said so is probably the worst misconception in all of physics. Consider Einstein's equivalence principle (weak form)spidey said:i don't understand uniform gravitational field and curvature is zero...how can a curvature be zero in uniform gravitational field...
If the spacetime is flat then it is impossible to introduce spacetime curvature by changing the spacetime coordinate from that of an inertial frame in a flat spacetime to coordinates corresponding to a uniformly accelerating frame of reference.A uniform gravitational field is equivalent to a uniformly accelerating frame of reference in flat spacetime.
The Christoffel symbols for an observer in a uniform gravitational field are non-zero. For this reason particles, as well as light, are deflected.One can always find in any given locality in which all local "gravitational fields" (all Christofell symbols: all \Gamma^{\alpha}_{\mu\nu}) disappear. No \Gamma means no "gravitational field" ...