抽象的
Essay on Calculating Dark Energy and Dark Matter
Friedhelm M. Joge*
A formula for calculating dark energy is established through derivation. The result is tested on the basis of the available data from the MAX PLANCK Institute for Radio Astronomy. The universe's dark matter has been computed. There is a balance sheet created and the most important formulas compiled. Summary: The rudiments of a theory of dark energy. The theoretical result is confronted with the numerical value calculated from the available data. Excellent matching of numerical values resulting in three independent paths makes the approach plausible. The approach is credible because of the excellent matching of numerical values that produces three separate routes. The task at hand is comparable to Kepler's planetary orbital rules. Only Isaac Newton gave Kepler's laws a theoretical foundation, which Thomass Gornitz provides here. Niels Bohr, who computed the energy levels of the hydrogen atom and the frequencies of spectral lines, theoretically supported the empirical Balmer formula for the spectral line frequencies in the arc spectrum of the hydrogen atom. A mysterious element known as dark energy is theorized to accelerate the universe's expansion by repelling matter. Theorists have proposed a variety of methods to calculate dark energy over the years. Numerous theories, however, fail to apply a metric structure to gravity or energy momentum conservation even when they satisfy strict local tests. The most popular option for dark energy is the cosmological constant, often known as vacuum energy density. By its very nature, dark energy is a low-energy phenomenon that is dispersed. It is not present in galaxies or galaxies in clusters and it is probably unlikely to be found in laboratory research. The repellent dark energy that hastens the universe's expansion could be explained if the cosmological constant is the vacuum energy of space. Nobody, however, is aware of the cosmological constant's existence or the amount that might be assigned to it in order to calculate the universe's acceleration. Any two matter fields can interact with each other in particle physics or on a more theoretical level, according to a possible process called the interaction of dark matter and dark energy. The phenomenological theory in question has aroused the interest of the cosmology community for a number of reasons. As in the interaction model, where dark energy decays into dark matter, interacting models of DM and DE are an equivalent description of the dark sector of the universe that have undergone extensive research and are motivated by a viable explanation to the socalled coincidence and cosmological constant concerns.
