How to measure dark energy?
In some models, the cosmic voids are forming dark energy. In that model, the quantum fields fall into that void and impact together in them. The cosmic void acts like a vacuum bomb.
This model means that there is a standing wave in the middle of those voids where quantum fields reflect. So what separates this thing from the gravitation? That is the wavelength of traveling electromagnetic fields and gravitation is one energy field.
In some other versions of this model, the cosmic voids increase the speed of material vaporization. In that process, the material turns into electromagnetic wave movement. When that wave movement hits to void's edge. This impact causes energy interaction called dark energy. But this is only a hypothesis.
So we must remember one thing. There must be many radiation wavelengths that are forming entireties called dark energy. Dark energy consists of multiple radiation wavelengths that are not visible to us or our sensors. In some models, dark energy is electromagnetic radiation that has a shorter wavelength than gamma radiation. And other side of the electromagnetic spectrum outside gravitational waves is another dark energy area.
"Using simulated data, astronomers have depicted the sky through gravitational waves, revealing the need for space observatories to detect binary systems. Future projects like LISA aim to uncover thousands of these hard-to-detect systems, marking a paradigm shift in space observation. (Artist’s illustration — see video below for simulation.)" (ScitechDaily.com/NASA’s Cosmic Vision: Simulating Our Galaxy Through Gravitational Waves)
The thing that could help to understand dark energy is to find out how it interacts with the environment. Does it interact straight with particles? Or does it interact with the particle's environment?
When researchers want to measure how much dark energy a system contains they must know how much visible energy is in the system. Then they must find some point that they use as the benchmark. After that researchers must calculate how that anomaly behaves if it contains only visible energy. Then they must just reduce those visible energy values from the values, that sensors give. And then we must strip dark energy out of those values.
Theoretically, that thing might seem very easy, but the problem is that dark- and visible energy affect the system together. The accuracy of the models depends on the knowledge of the system. Researchers should separate the values that visible energy gives. From the values that the dark energy and visible energy give together. And the problem is that nobody measured dark energy. Accurate calculations require the knowledge of the power of dark energy.
But there is no quantum-scale observation from dark energy. Dark energy is visible only in large-scale systems. There is a vision that dark energy is energy that travels out from material because of cosmic expansion. In some other visions, at least part of dark energy is energy. That comes out from black holes. In that model, there are many types of dark energy. And electromagnetic spectrum continues far away from gamma- and from other side radio waves. So is there an endless number of wavelengths in the electromagnetic spectrum?
When we are talking about visible energy, that thing contains many types of radiation. Gravitational waves, X, and gamma-rays are also "visible energy". And maybe we should stop thinking that things like dark energy or gravitational waves have only one wavelength. There could be many wavelengths that form gravitational waves and dark energy. So that means those energy waves can affect different points in the particles and their environment.
That means there might be two effects that we call as gravitational effect. The first interacts straight with the particle. The second interacts with the particle through its environment. In the first version, the superstring that forms the particle's spinning shell cuts the gravitational superstring. In the second model quantum fields that travel in some kind of electromagnetic vacuum pull particles in the gravitational center.
In some visions the black holes or their singularity spins very fast. And that interaction drives quantum fields into its poles. Then quantum field travels to that extremely dense object's poles plus the other quantum fields through the event horizon and those quantum fields pull other particles with them.
The wavelength of the gravitational waves is thousands or even millions of kilometers. There is the possibility that gravitational interaction happens when a gravitational wave travels through the spinning particles. The spinning part is the whisk-looking superstring structure, and the gravitational wave is like a string that travels through this structure. When the superstring hits the gravitational waves it harvests energy in it.
So if we think that gravitational waves have multiple wavelengths there is the possibility that some gravitational waves are forming an electromagnetic vacuum that causes the effect, where falling quantum fields try to fill that bubble. And those electromagnetic fields or quantum fields are pulling particles with them.
We can see short-wave gamma- and long-wave radio waves. The gravitational waves can be thousands or even millions of kilometers long. And that makes it hard to detect them. In some models, all black holes send gravitational waves with their unique wavelengths.
That depends on the event horizon's size. In that model, the dense energy between the transition disk and the event horizon is the point, where gravitational waves are leaving. In that case, the dense energy interacts with quantum fields sending radiation that we know as gravitational waves.
https://scitechdaily.com/cambridge-researchers-discover-new-way-to-measure-dark-energy/
https://scitechdaily.com/nasas-cosmic-vision-simulating-our-galaxy-through-gravitational-waves/
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