期刊文献+
共找到9篇文章
< 1 >
每页显示 20 50 100
Dark Matter Creation and Anti-Gravity Acceleration of the Expanding Universe
1
作者 F. C. Hoh 《Journal of Modern Physics》 2021年第3期139-160,共22页
Dark matter is identified as negative relative energy between quarks in proton and is generated in cold hydrogen gas with pressure gradient in gravitational field. Positive relative energy PRE can be generated between... Dark matter is identified as negative relative energy between quarks in proton and is generated in cold hydrogen gas with pressure gradient in gravitational field. Positive relative energy PRE can be generated between quarks in protons in cold hydrogen gas in outskirts of the universe. The mechanisms for such creation of dark matter and PRE are reviewed and updated in greater detail and clearer manner. The so-generated dark matter in a galaxy can account for the galaxy’s rotation curve. Star formation in this galaxy uses up the hydrogen atoms and thereby reduces its dark matter content. Dark matter created in intergalactic hydrogen gas can form filaments. In a hypothetical model of the universe, a hydrogen atom with a small amount of negative relative energy or dark matter at the outskirts of this universe can via collisions with other atoms turn into one with a small positive relative energy PRE. Once such a sign change takes place, gravitational attraction switches to anti-gravity repulsion unopposed by any pressure gradient. This leads to a “run away” hydrogen atom moving away from the mass center of the universe and provides a basic mechanism for the accelerating expansion of the universe. This theoretical expansion and the measured redshift data are both compatible with the conception of an acceleratingly expanding universe and complement each other. But they cannot verify each other directly because the present model has been constructed for purposes different from those of the measurements. But it can be shown that both approaches do support each other qualitatively under certain circumstances for small velocities. Dark matter and PRE in the present model are not foreign objects like WIMPs and dark energy-cosmological constant but can only be created in cold hydrogen gas in gravitational field. To achieve this, infrequent collisions among the hydrogen atoms must take place. Dark matter was created first and can eventually later evolve into PRE in the outskirts of the universe and in the intergalactic void. Dark matter and PRE will disappear if the hydrogen atom carrying them becomes ionized as in stars. 展开更多
关键词 Relative Energy between Quarks Scalar Strong Interaction Hadron Theory SSI Negative Relative Energy Dark Matter Positive Relative Energy PRE Anti-Gravity Repulsion Universe Expansion Proton Orbit Hubble’s Law
下载PDF
On Excited Meson Spectra in the Scalar Strong Interaction Hadron Theory
2
作者 F. C. Hoh 《Journal of Modern Physics》 2017年第8期1127-1133,共7页
Meson spectra have been treated earlier in the scalar strong interaction hadron theory, choosing the Coulomb and linear type of potentials, neglecting the quadratic one. The spectra of ground state pseudoscalar and ve... Meson spectra have been treated earlier in the scalar strong interaction hadron theory, choosing the Coulomb and linear type of potentials, neglecting the quadratic one. The spectra of ground state pseudoscalar and vector mesons were adequately accounted for but not that of the excited mesons. Here, the quadratic potential replaces the Coulomb one and the same ground state meson spectra were recovered. Also, the masses of low-lying radially excited pseudoscalar and vector mesons were found to be 4% - 18% smaller than the measured ones. Here, the linear type of potential, by itself of nonlinear nature, has been neglected. For some orbitally excited pseudoscalar mesons, the difference is 14% - 38%. The discrepancies are tentatively attributed to the neglected nonlinear potential, which is expected to increase with meson mass, as can be seen in the tables below. 展开更多
关键词 EXCITED MESON Spectra QUADRATIC CONFINEMENT SCALAR Strong Interaction
下载PDF
On Dineutron and Deuteron Binding Energies
3
作者 F. C. Hoh 《Journal of Modern Physics》 2021年第3期161-166,共6页
The binding energy of the deuteron is estimated from the scalar strong interaction hadron theory SSI. The predicted value is 7.7% lower than the measured value. Existence of a spin 1 dineutron with a binding energy 4/... The binding energy of the deuteron is estimated from the scalar strong interaction hadron theory SSI. The predicted value is 7.7% lower than the measured value. Existence of a spin 1 dineutron with a binding energy 4/5 that of the deuteron or 1.78 MeV is predicted. This is verified by the dineutron, first observed in 2012, in <sup>16</sup>Be decay. No free dineutrons are expected to exist in nature as they can decay into deuterons. These binding energies are limited by short range strong interaction internucleon forces but consist of long range electrostatic energies from quark charges. 展开更多
关键词 Scalar Strong Interaction Hadron Theory SSI Deuteron Structure Dineutron Structure Electromagnetic Energy Deuteron Binding Energy Dineutron Binding Energy Dineutron Decay
下载PDF
On the Ratios Dark Matter (Energy)/Ordinary Matter ≈5.4(13.6) in the Universe
4
作者 F. C. Hoh 《Journal of Modern Physics》 2020年第7期967-975,共9页
An upper limit of the average ratio dark matter/ordinary matter in galaxies is estimated to be 8.4, in agreement with the observed ratio 5.4. Upper limit of the average ratio dark energy/ordinary matter for slowly mov... An upper limit of the average ratio dark matter/ordinary matter in galaxies is estimated to be 8.4, in agreement with the observed ratio 5.4. Upper limit of the average ratio dark energy/ordinary matter for slowly moving protons in the outer parts of the universe is estimated to be 8.4, much less than the observed ratio 13.6. The discrepancy is tentatively attributed to that the bulk of the protons in these outer parts of the universe moves fastly and their contribution to dark energy has not been estimated. The positive and negative relative energies between the diquark and quark in the proton play the roles of dark energy and dark matter, respectively. 展开更多
关键词 Relative Energy Between Quarks Scalar Strong Interaction Hadron Theory Ratio of Dark Matter to Ordinary Matter Ratio of Dark Energy to Ordinary Matter Gravitational Pull of Diquark and Quark Proton Orbit Diquark Equations
下载PDF
CP Violation in Kaon Decay in the Scalar Strong Interaction Hadron Theory
5
作者 F. C. Hoh 《Journal of Modern Physics》 2012年第10期1562-1571,共10页
CP conservation and violation in neutral kaon decay are considered from a first principles’ theory, recently published as “Scalar Strong Interaction Hadron Theory”. The arbitrary phase angle relating K0 and 0 in cu... CP conservation and violation in neutral kaon decay are considered from a first principles’ theory, recently published as “Scalar Strong Interaction Hadron Theory”. The arbitrary phase angle relating K0 and 0 in current phenomenology is identified to be related to the product of the relative energy to the relative time between the s and d quarks in these kaons. The argument of the CP violating parameter ? is predicted to be 45? without employing measured data. The K0S decay rate is twice the K0L -K0S masss difference, in near agreement with data, and both are proportional to the square of the relative energy 29.44 eV. Any pion from K0L decay will also have a mass shift of ≈1.28 × 10-5 eV. The present first principles’ theory is consistent with CP conservation. To achieve CP violation, the relative time cannot extend to both +∞ and -∞ but is bounded in at least one direction. The values of these bounds lie outside the present theory and it is unknown how they can be brought forth. -B0 mixing is also considered and the relative energy is 663.66 eV. 展开更多
关键词 CP VIOLATION KAON DECAY RELATIVE Energy RELATIVE Time SCALAR Strong Interaction
下载PDF
QCD as High Energy Limit of the Scalar Strong Interaction Hadron Theory
6
作者 F. C. Hoh 《Journal of Modern Physics》 2013年第9期1171-1175,共5页
This paper is an extension of the book of reference [1] below. QCD Lagrangian is derived from the same equations of motion for quarks used to construct the equations of motion for mesons and baryons in the scalar stro... This paper is an extension of the book of reference [1] below. QCD Lagrangian is derived from the same equations of motion for quarks used to construct the equations of motion for mesons and baryons in the scalar strong interaction hadron theory that accounts for many basic low energy data not covered by QCD. At high energies, the energetic quarks in a hadron can be far from each other and approximately free. Each quark is associated with a vector in an internal space characterizing its mass and charge. These spaces are interchangeable and provide a new symmetry equivalent to color symmetry in QCD. A quark in a meson has two “colors” and in a baryon three “colors”;the β function of QCD is 61%-92% greater in high energy interactions leading to baryons than that to mesons. This function enters the measurable running coupling constant and this prediction is testable against experiment. QCD, successful at high energies, is thus reconciled with the scalar strong interaction hadron theory and both complement each other. 展开更多
关键词 QCD at High ENERGIES SCALAR Strong Interaction Internal SYMMETRY
下载PDF
Baryon Magnetic Moment in the Scalar Strong Interaction Hadron Theory
7
作者 F. C. Hoh 《Journal of Modern Physics》 2014年第11期995-1000,共6页
The magnetic moments of the baryon octet are derived from a first principle’s theory, the scalar strong interaction hadron theory, and are in approximate agreement with data. It is conjectured that this agreement may... The magnetic moments of the baryon octet are derived from a first principle’s theory, the scalar strong interaction hadron theory, and are in approximate agreement with data. It is conjectured that this agreement may be improved by including the “spin-orbit coupling” term not evaluated here. 展开更多
关键词 BARYON Magnetic MOMENT First Principle’s THEORY Internal COORDINATES
下载PDF
Higgs-Like Boson and Bound State of Gauge Bosons W+W-
8
作者 F. C. Hoh 《Journal of Modern Physics》 2016年第1期36-42,共7页
The Higgs-like boson H(126) discovered in 2012 is tentatively assigned to a newly found bound state of two charged gauge bosons W<sup>+</sup>W<sup>-</sup>. Starting from the scalar strong inter... The Higgs-like boson H(126) discovered in 2012 is tentatively assigned to a newly found bound state of two charged gauge bosons W<sup>+</sup>W<sup>-</sup>. Starting from the scalar strong interaction hadron theory, a first principles’ theory, a nonlinear, soliton-like differential equation dependent upon the distance between the two W bosons is derived. This equation is solved on a computer. A new, nonlinear confinement mechanism, not yet understood, binds the both bosons and gives a bound state mass E<sub>B</sub> = 155.8 GeV. This E<sub>B</sub>, derived at the quantum mechanical level, is estimated to reduce to E<sub>B</sub> = 110 GeV when quantized field effects are included via coarse approximations and replacement of the bare constants by renormalized ones. These developments lead to a revised status of the standard model. 展开更多
关键词 Bound State of W+W- Scalar Strong Interaction Soliton-Like Equation
下载PDF
Higgs-Like Boson and Bound State of Gauge Bosons W+W- II
9
作者 F. C. Hoh 《Journal of Modern Physics》 2016年第11期1304-1307,共4页
The Higgs-like boson discovered at CERN in 2012 is tentatively assigned to a newly found bound state of two charged gauge bosons W<sup>+</sup>W<sup>-</sup> with a mass of E<sub>B</sub&... The Higgs-like boson discovered at CERN in 2012 is tentatively assigned to a newly found bound state of two charged gauge bosons W<sup>+</sup>W<sup>-</sup> with a mass of E<sub>B</sub> ≈ 117 GeV, much closer to the measured 125 GeV than 110 GeV predicted in a paper with the same title earlier this year. The improvement is due to a shift from the earlier SU(2) representation assignment for the gauge bosons to the more realistic SU(3) one and that the computations are carried out with much greater accuracy. 展开更多
关键词 Bound State of W+W- Higgs-Like Boson SU(3) Group
下载PDF
上一页 1 下一页 到第
使用帮助 返回顶部