Initial recognition for rolling waves in 2016 he provided a definitive confirmation of Einstein’s theory of relation. But some strange predictions have not been confirmed: According to the obvious connection, each gravitational force must leave an indelible mark on the structure of the atmosphere. It should disturb the space permanently, and remove the mirrors of the lighting fixture even after the waves have passed.
Ever since the first discovery about six years ago, scientists have been trying to figure out how to test what is called “memory memory.”
“Memory is a strange, strange thing,” he said Paul Lasky, an astronomer at Monash University in Australia. “It’s a very deep thing.”
Their goal is greater than simply looking at the permanent scars left in the sky by the force of gravity passing through them. In their study of the relationship between objects, energy, and time in space, astronomers look forward to a better understanding of Stephen Hawking’s. disturbing knowledge of the black hole, which has been the focus of 50 years of psychological research. “There is a strong correlation between memory retrieval and the parallelity of space time,” he said Kip Thorne, a scientist at the California Institute of Technology whose work on gravitational waves made him a part of 2017 Nobel Prize in Physics. “It is connected at the end with the loss of knowledge in the black holes, a very serious matter in the design of space and time.”
A Scar in Spacetime
Why can strong currents really change the atmosphere? It drops to the intermediate connection of space time and energy.
First, consider what happens when a powerful wave passes through a magnetic field. The Laser Interferometer Gravitational-Wave Observatory (LIGO) has two arms in the shape of L. If you think the circle is around the arms, and in the middle of the circle at the intersection of the arms, the force of gravity periodically distorts the circle, until the waves pass over. The long difference between the two arms will rotate — systems that show the curve of the circle, and the passage of strong gravitational waves.
According to memory recall, after passing the waves, the circle should be permanently deformed with a small density. The reason has to do with the way gravity is defined by relativity.
The things that LIGO realizes are so far away, their gravitational pull is so weak. But gravity has a longer duration than gravity. Likewise, the thing that triggers memory memory: gravity.
In Newtonian’s simple terms, gravity measures the amount of force an object can receive if it falls from a certain distance. Dropping a storm on a rock, and the speed of an eagle on the ground can be used to recreate the “possible” forces that can fall on a rock.
But in normal relationships, when air time is stretched and broken up in different directions depending on how the bodies move, the potential simply refers to the energy that can be in place – it depends on the shape of the atmosphere.
“Memory is nothing but a change in gravity,” Thorne said, “but it is a gravitational pull.” Transmitting force causes a change in gravity; This change is time consuming, even when the waves are passing.
How can a passing wave affect time? The possibilities are endless, and, surprisingly, these possibilities are the same. In this way, space time is like Boggle’s unlimited game. Boggle’s premium game consists of 16 six-dimensional dice arranged in a four-grid, with characters on each side of the die. Each time a player shakes the board, the dice roll around and settle in a new alphabet. Many changes are different from each other, but they are all the same in a great sense. They are all at rest in the lowest energy that dice can hold. As the gravitational force passes, it shakes the cosmic Boggle board, changing the space from one wonky shift to another. But space time remains a very small force.
That culture – that you can change the board, but in the end things stay the same – indicates the presence of hidden symmetries in the time structure. In the last decade, scientists have made that connection.
The story began in the 1960s, when four astronomers sought to better understand common sense. They wondered what would happen to the imaginary region that is far away from the natural forces of nature, where the earth’s gravitational pull would be ignored, but gravity would not. He started by looking at the symmetries that the region listens to.