We investigate the fabric of spacetime, its ability to stretch, curve, and expand. Through our continuous studies of accretion disks located at the core of galaxies, it is our conclusion that these disks are separate from the host galaxy stellar disk.

The Final Size of the Universe Based on the Elasticity of the Fabric of Spacetime
     Geo Douglas1*, Naman S. Bajaj2

Our research has also determined that the radius of accretion disks in spiral galaxies follow a consistent ratio according to the circumference of their adjacent supermassive black hole based on its Schwarzchild radius. We present evidence suggesting that galactic accretion disks are a key element to understand galaxy formation and can provide a precise calculation to how much the fabric of space will stretch. Once the degree of the elasticity of spacetime was established, we applied these measurements to the size of the universe at 380,000 years of age based on the imagery of the cosmic microwave background. This calculation provided us with the maximum diameter the universe will reach, an exact time when the universe will stop expanding, and where we are today within that timeline.

https://www.scirp.org/journal/paperinformation?paperid=101773

SEE ALSO an old article:

The collision of distant black holes generates gravitational waves, or ripples in 'space-time'. Space-time can be thought of as a 'fabric' in which the objects of the Universe are embedded.

Those objects - stars, planets, black holes - make space-time curve in upon itself, just as an elastic fabric holding a ball would do. The more massive the object, the deeper the curve - the same as in a fabric!

This is, at least, what Albert Einstein wrote more than eight decades ago. Many of the predictions derived from his theory have been proven already, but not all. For example, Einstein predicted that if two very massive bodies moved, they would cause 'ripples' in the space-time continuum; moreover, those ripples would propagate at the speed of light, alternately stretching and squeezing space.

These waves, called gravitational waves, have never been physically detected. The technology to do it has simply not been available, until now.

ESA's mission LISA, scheduled for launch in 2012, aims to detect gravitational waves. It will be a new way to 'sense' the Universe. By perceiving the movement of very massive objects within a radius of thousands of millions of light-years, we will be able to detect some of the most amazing events in the Universe, such as the collision of two distant black holes.

LISA Pathfinder, due for launch in 2007, will demonstrate the technology needed for LISA, one of ESA's future missions.

https://www.esa.int/Science_Exploration/

Space_Science/Space-time_as_an_elastic_fabric

SEE ALSO: https://www.youtube.com/watch?v=luvf_9EaJ0w

FREE JULIAN ASSANGE NOW, PLEASE..........