Physics Maths Engineering
Helena Drueke,
Helena Drueke
Institution: Institute of Physics, University of Rostock, 18051 Rostock, Germany
Email: helena.drueke@uni-rostock.de
Dieter Bauer
Dieter Bauer
Institution: Institute of Physics, University of Rostock, 18051 Rostock, Germany
Email: dieter.bauer@uni-rostock.de
"Periodic driving may cause topologically protected, chiral transport along edges of a 2D lattice that, without driving, would be topologically trivial. We study what happens if one adds a different on-site potential along the diagonal of such a 2D grid. In addition to the usual bulk and edge states, the system then also exhibits doublon states, analogous to two interacting particles in one dimens...
2 years ago
Physics Maths Engineering
Meir Shimon
Meir Shimon
Institution: School of Physics and Astronomy, Tel Aviv University,
Email: meirs@tauex.tau.ac.il
In the standard cosmological model the dark energy (DE) and nonrelativistic (NR) matter densities are determined to be comparable at the present time, in spite of their greatly different evolution histories. This ‘cosmic coincidence’ enigma could be explained as a non-anthropic observational selection effect: We show that in a suitably chosen frame the Universe is at its most probable epoch wh...
2 years ago
Physics Maths Engineering
Oleg Lebedev,
Oleg Lebedev
Institution: Department of Physics and Helsinki Institute of Physics, Gustaf Hallstromin katu 2a, FI-00014
Email: info@res00.com
Jong-Hyun Yoon
Jong-Hyun Yoon
Institution: Department of Physics and Helsinki Institute of Physics, Gustaf Hallstromin katu 2a, FI-00014
Email: info@res00.com
We consider dark matter production during the inflation oscillation epoch. It is conceivable that renormalizable interactions between dark matter and inflation may be negligible. In this case, the leading role is played by higher dimensional operators generated by gravity and thus suppressed by the Planck scale. We focus on dim-6 operators and study the corresponding particle production in perturb...
2 years ago
Physics Maths Engineering
Joseph E Brierly
Joseph E Brierly
Institution: Joseph E Brierly, Ph.D., Wayne State University,
Email: jbrierly@comcast.net
This article gives a overall picture of how the universe works from the likelihood that our universe is infinite dimensional at the nanometer scale of an indestructible quark. The article explains that we only can perceive for sure up to 4 dimensions of physical reality. However, the speculation in this article seems very clear that likely we are seeing activity in the 5th dimension in particle ph...
2 years ago
Physics Maths Engineering
Robert J Buenker Buenker
Robert J Buenker Buenker
Institution: Faculty of C-Mathematics and Natural Sciences, Bergische Universität Wuppertal,
Email: rjbuenker@gmail.com
A number of the most often cited results of relativity theory deal with the relationships between energy, momentum and inertial mass. The history of how Einstein and Planck came to these conclusions is reviewed. It is pointed out that considerations of how the speed of light is affected by the motion of the Earth played a determining role in these developments. After the Michelson-Morley null-inte...
2 years ago
Physics Maths Engineering
Berov G Lyubomir
Berov G Lyubomir
Institution: Engineer, Independent Innovative Ideas Researcher, Smolyan 4700,
Email: my_kaly1@mbox.contact.bg
The present, at any particular moment, is the realization of one of the many intentions of the All-creating Intellect. Here "realization" specifically means the materialization or the appearance of an object in the material world, which had not existed until now. This newly born material object exists only for the duration of the moment of "now". This moment is infinitely short, or, if we use a co...
2 years ago
Physics Maths Engineering
It is widely believed that Hawking radiation originates from excitations near the horizons of black holes [1,2,3]. However, Giddings [2] proposed that the Hawking radiation spectrum that characterizes evaporating semi-classical black holes originates from a quantum “atmosphere”, which extends beyond the horizon of a black hole. Although several research projects have been conducted in this fie...
3 years ago
Physics Maths Engineering
Kamila Sieja
Kamila Sieja
Institution: Institute Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (CNRS, UMR7178),
Email: la.sieja@iphc.cnrs.fr
Neutron-rich Sr nuclei around N = 60 exhibit a sudden shape transition from a spherical ground state to strongly prolate-deformed. Recently, much new insight into the structure of Sr isotopes in this region has been gained through experimental studies of the excited levels, transition strengths, and spectroscopic factors. In this work, a “classic” shell model description of strontium
isotopes...
3 years ago
Physics Maths Engineering
In this paper we consider the correspondence between the tachyon dark energy model and the Tsallis holographic dark energy scenario in an FRW universe. We demonstrate the Tsallis holographic description of tachyon dark energy in an FRW universe and reconstruct the potential and basic results of the dynamics of the scalar field which describe the tachyon cosmology. In a flat universe, in the tachyo...
3 years ago
Physics Maths Engineering
Anand K. Bhatia
Anand K. Bhatia
Institution: Heliophysics Science Division, NASA/Goddard Space Flight Center,
Email: d.k.bhatia@nasa.gov
The excitation cross-sections of the nS states of atomic hydrogen, n = 2 to 6, by electron
impact on the ground state of atomic hydrogen were calculated using the variational polarizedorbital method at various incident electron energies in the range 10 to 122 eV. Converged excitation
cross-sections were obtained using sixteen partial waves (L = 0 to 15). Excitation cross-sections to
2S state, ...
3 years ago