Planck Mass Rotons as Cold Dark Matter and Quintessence*
... They are: 1. About 70% of the material content of the universe is a negative pressure energy, 2. About 26% nonbaryonic cold dark matter, 3. About 4% ordinary matter and radiation, 4. The universe is Euclidean flat, 5. It’s cosmological constant very small, 6. It’s expansion slightly accelerated. The ...
... They are: 1. About 70% of the material content of the universe is a negative pressure energy, 2. About 26% nonbaryonic cold dark matter, 3. About 4% ordinary matter and radiation, 4. The universe is Euclidean flat, 5. It’s cosmological constant very small, 6. It’s expansion slightly accelerated. The ...
The interpretation of the Einstein-Rupp experiments and their
... Einstein and Rupp’s Grid Experiment (“I would like to add some comments that connect to the problem that you have recently discussed in the Proceedings of the Berlin Academy.”) 24 After first arguing that the concept of a finite wave train was in good agreement with the uncertainty principle for qua ...
... Einstein and Rupp’s Grid Experiment (“I would like to add some comments that connect to the problem that you have recently discussed in the Proceedings of the Berlin Academy.”) 24 After first arguing that the concept of a finite wave train was in good agreement with the uncertainty principle for qua ...
The purpose of this course is to introduce the key
... 132. Explain how atomic spectra provide observational evidence for quantum theory. Why does hot hydrogen gas only emit certain discrete colors (spectral lines)? 133. Explain how the spectrum emitted by hydrogen provides information about the energy levels of electrons in hydrogen gas. 134. Explain ...
... 132. Explain how atomic spectra provide observational evidence for quantum theory. Why does hot hydrogen gas only emit certain discrete colors (spectral lines)? 133. Explain how the spectrum emitted by hydrogen provides information about the energy levels of electrons in hydrogen gas. 134. Explain ...
Notes14
... also present. That is, work is done to move the mass from its equilibrium state (giving it potential energy), then a restoring force pulls it back toward its equilibrium state. In the case of pendulum-like motion (which occurs in some form or another in almost all physical systems), momentum and kin ...
... also present. That is, work is done to move the mass from its equilibrium state (giving it potential energy), then a restoring force pulls it back toward its equilibrium state. In the case of pendulum-like motion (which occurs in some form or another in almost all physical systems), momentum and kin ...
