期刊文献+
共找到314篇文章
< 1 2 16 >
每页显示 20 50 100
The Reality of Baryonic Acoustic Oscillations
1
作者 J. C. Botke 《Journal of Modern Physics》 2024年第3期377-402,共26页
The initial idea for baryonic acoustic oscillations (BAO) came about during early efforts to understand the origin of galaxies by studying perturbed versions of the Friedmann-Robertson-Walker (FRW) model. In more rece... The initial idea for baryonic acoustic oscillations (BAO) came about during early efforts to understand the origin of galaxies by studying perturbed versions of the Friedmann-Robertson-Walker (FRW) model. In more recent times, the emphasis has shifted to the idea that 2-point galaxy correlations embedded in the distribution of matter by the BAO could be used as a standard ruler to fix the parameters of cosmological models. In this paper, we first consider the actual business of extracting the correlation length from large data sets of measured galaxy locations. To facilitate this process, we introduce a much-improved method for extracting the correlation peak from the data set. Fundamental to this process in any model is the use of a fiducial cosmological model to transition from redshift space to comoving coordinate space where the correlations actually exist. The belief is that the correlation length so determined can then be reverted to redshift space to fix the parameters of cosmological models. We show, however, that this process is circular and hence of no value whatsoever for fixing model parameters. All one obtains are the parameters of the model used to transition to comoving space in the first place. Finally, we present simple arguments that show that the idea of BAO being responsible for the structure of the universe, i.e. the cosmic web, is unworkable. 展开更多
关键词 baryonic Acoustic Oscillations Two-Point Correlations CMB Anisotropy Early Universe Time-Varying Curvature
下载PDF
Describing a Baryon as a Meson Pair
2
作者 Teruo Kurai 《Journal of Modern Physics》 2020年第11期1827-1841,共15页
We propose a new description of a baryon as a pair of mesons. This description is an extension of the previously proposed description of a nucleon as a pair of pions. The purpose of this article is to show the followi... We propose a new description of a baryon as a pair of mesons. This description is an extension of the previously proposed description of a nucleon as a pair of pions. The purpose of this article is to show the following two possibilities. The first one is that it shows the qualitative explanation to support our description of a nucleon as a pair of pions and the second one is that it gives the systematic way of estimation of baryon mass not only for light baryons but also for heavy baryons (charm baryons and bottom baryons). Each isospin group is constructed of both baryons and antibaryons. This way of construction is consistent with that of mesons. The results obtained are listed in tables (Tables 1-9). This shows that the generalized Gell-Mann-Nishijima relation equation holds under the condition that the baryon number is 0 and that the obtained masses are fairly good, even for heavy baryons. Our description also yields several examples of baryon decay modes. 展开更多
关键词 baryon Description baryon Isospin baryon Mass baryon Decay Mode
下载PDF
The Periodic Table of Elementary Particles for Baryonic Matter and Dark Matter: Upward-Going ANITA Events
3
作者 Ding-Yu Chung 《Journal of Modern Physics》 2018年第13期2308-2319,共12页
This paper posits that the upward-going ANITA events are derived from the cosmic ray of the baryonic-dark matter (BDM) Higgs boson. In the extended standard model (ESM) for baryonic matter and dark matter, the spontan... This paper posits that the upward-going ANITA events are derived from the cosmic ray of the baryonic-dark matter (BDM) Higgs boson. In the extended standard model (ESM) for baryonic matter and dark matter, the spontaneous symmetry breaking through the Higgs mechanism for the symmetrical massless baryonic matter left-handed neutrinos and massless dark matter right-handed neutrinos produced massless baryonic matter left-handed neutrinos, sterile massive dark matter neutrinos, and the BDM Higgs boson. The BDM Higgs boson is the composite of the high-mass tau neutrino and the high-mass dark matter neutrino. During the passage through the high-density part of the Earth, the BDM Higgs boson is transformed into the oscillating BDM Higgs boson between the composite of the high-mass tau neutrino and the high-mass dark matter neutrino and the composite of the high-mass tau neutrino and the low-mass dark matter neutrino. The oscillating BDM Higgs boson decays into the high-mass tau neutrino with the extra energy and the low-mass dark matter neutrino (27 eV) in the low-density water-ice layer of the Earth. The high-mass tau neutrino is converted into ultra-high-energy tau neutrino which decays into tau lepton through the charged-current interactions, and tau lepton emerges from the surface of ice. Based on the periodic table of elementary particles, the calculated value for the high-mass tau neutrino with the extra energy is 0.47 EeV in good agreement with the observed 0.56 and 0.6 EeV. The periodic table of elementary particles for baryonic matter, dark matter, and gravity is based on the seven principal mass dimensional orbitals for stable baryonic matter leptons (electron and left-handed neutrinos), gauge bosons, gravity, and dark matter and the seven auxiliary mass dimensional orbitals for unstable leptons (muon and tau) and quarks, and calculates accurately the masses of all elementary particles and the cosmic rays by using only five known constants. 展开更多
关键词 ANITA Periodic Table of Elementary Particles HIGGS BOSON baryonic-Dark MATTER HIGGS BOSON Cosmic RAYS Upward-Going DARK MATTER baryonic MATTER Extended Standard Model
下载PDF
Baryon wave functions and free neutron decay in the scalar strong interaction hadron theory (SSI)
4
作者 F. C. Hoh 《Natural Science》 2010年第9期929-947,共19页
From the equations of motion for baryons in the scalar strong interaction hadron theory (SSI), two coupled third order radial wave equations for baryon doublets have been derived and published in 1994. These equations... From the equations of motion for baryons in the scalar strong interaction hadron theory (SSI), two coupled third order radial wave equations for baryon doublets have been derived and published in 1994. These equations are solved numerically here, using quark masses obtained from meson spectra and the masses of the neutron, ?0 and ?0 as input. Confined wave functions dependent upon the quark-diquark distance as well as the values of the four integration constants entering the quark-diquark interaction potential are found approximately. These approximative, zeroth order results are employed in a first order perturbational treatment of the equations of motion for baryons in SSI for free neutron decay. The predicted magnitude of neutron’s half life agrees with data. If the only free parameter is adjusted to produce the known A asymmetry coefficient, the predicted B asymmetry agrees well with data and vice versa. It is pointed out that angular momentum is not conserved in free neutron decay and that the weak coupling constant is detached from the much stronger fine structure constant of electromagnetic coupling. 展开更多
关键词 SCALAR Strong Interaction baryon Radial Wave Functions Free NEUTRON DECAY
下载PDF
Experimental Evidence of Non-Baryonic Dark Matter in High Energy Physics 被引量:2
5
作者 Matsuo Sekine 《Journal of High Energy Physics, Gravitation and Cosmology》 2021年第3期873-879,共7页
If most of the universe is made of baryons, we encounter a serious contradiction in explaining the observed structure formulation. Therefore, we need non-baryonic dark matter to comprise the universe. In a previous pa... If most of the universe is made of baryons, we encounter a serious contradiction in explaining the observed structure formulation. Therefore, we need non-baryonic dark matter to comprise the universe. In a previous paper, the present author proposed an infinite sub-layer quark model in which there exists an infinite number of up quark <i>q<sub>u</sub></i> (∞) and down quark <i>q<sub>d</sub></i> (∞) at an infinite sub-layer level. These quarks have non-baryon quantum number with one-half electric charge. Thus, <i>q<sub>u</sub></i> (∞) and <i>q<sub>d</sub></i> (∞) quarks are candidates for the non-baryonic dark matter. It is then shown that CP is violated only in the doublet of <i>q<sub>u</sub></i> (∞) and <i>q<sub>d</sub></i> (∞) quarks to account for the asymmetry of the number of particles and anti-particles in the present universe. It should be emphasized that if the internal space of <i>q<sub>u</sub></i> (∞) and <i>q<sub>d</sub></i> (∞) quarks in the first generation is a noncommutative geometry, CP violation can be explained without increasing the number of particles and generations. Thus, a pair of an infinite number of <i>q<sub>u</sub></i> (∞) and <i>q<sub>d</sub></i> (∞) quarks would be produced in the first moments after the Big Bang and form the hadrons including the nucleons and remain as the non-baryonic cold dark matter for all time. From the <i>q<sub>f</sub></i> (∞) quarks with the flavors <i>f</i> = <i>u</i>, <i>d</i>, <i>s</i>, <i>c</i>, <i>t</i>, and <i>b</i>, we compared our prediction value of the cross-section ratio <i>R</i> with the experimental values. We obtained the theoretical branching ratio <i>R</i> = 15/4 = 3.75 which is in good agreement with the experimental values from 12.00 GeV to 46.47 GeV in electron-positron annihilation into muon pairs and quark pairs. 展开更多
关键词 Non-baryonic Dark Matter Non-baryonic Quark Electron-Positron Annihilation
下载PDF
The Cosmological Evolution of Baryonic Matter’S Density Perturbations Under Influence of the Quintessence
6
作者 Chechin Leonid Mikhajlovich 《Journal of Modern Physics》 2011年第8期834-840,共7页
For deeper understanding the process of baryonic matter evolution in the expanding Universe it is necessary to know the physical property of concrete field that represents the background of substrate type of dark ener... For deeper understanding the process of baryonic matter evolution in the expanding Universe it is necessary to know the physical property of concrete field that represents the background of substrate type of dark energy. Beside, it is necessary to explore in details the influence of such field on the continuous medium of baryonic matter. These statements were realized for the quintessence field that describes by two gravitating scalar fields. They give own contributions at the total pressure and at the total mass density of baryonic matter. It allowed show that evolution of baryonic matter’s density perturbations obeys the equation of forced oscillations and admits the resonance case, when amplitude of baryonic matter’s density perturbations gets the strong short-time splash. This splash interprets as a new macroscopic mechanism of the initial matter density perturbations appearance. 展开更多
关键词 baryonic Matter’S Density PERTURBATIONS QUINTESSENCE Field NONSTATIONARY EQUATION Of State Of The UNIVERSE
下载PDF
Holography, Charge, and Baryon Asymmetry
7
作者 T. R. Mongan 《Journal of Modern Physics》 2012年第7期581-584,共4页
The reason for baryon asymmetry in our universe has been an open question for many years. This note shows that the holographic principle requires a charged preon model underlying the Standard Model of particle physics... The reason for baryon asymmetry in our universe has been an open question for many years. This note shows that the holographic principle requires a charged preon model underlying the Standard Model of particle physics and, in consequence, requires baryon asymmetry. The baryon asymmetry predicted by a specific charged preon model in our closed inflationary Friedmann universe is consistent with observations. 展开更多
关键词 baryon Asymmetry CHARGED Preon Models HOLOGRAPHIC PRINCIPLE
下载PDF
Baryon Magnetic Moment in the Scalar Strong Interaction Hadron Theory
8
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
Investigation and Study of the Effects of Hyperfine Interaction on the Mass of Baryons N and Δ
9
作者 Alireza Heidari Seyedali Vedad Mohammadali Ghorbani 《Journal of Modern Physics》 2012年第6期492-495,共4页
The following article has been retracted due to the investigation of complaints received against it. Mr. Mohammadali Ghorbani (corresponding author and also the last author) cheated the authors’ name: Alireza Heidari... The following article has been retracted due to the investigation of complaints received against it. Mr. Mohammadali Ghorbani (corresponding author and also the last author) cheated the authors’ name: Alireza Heidari and Seyedali Vedad. The scientific community takes a very strong view on this matter and we treat all unethical behavior such as plagiarism seriously. This paper published in Vol.3 No.6 492-495, 2012, has been removed from this site. 展开更多
关键词 baryon SPIN ISOSPIN Schr?dinger EQUATION HYPERFINE Interaction
下载PDF
Study of Baryon Acoustic Oscillations with SDSS DR13 Data and Measurements of &Omega;<sub>k</sub>and &Omega;<sub>DE</sub>(a)
10
作者 B. Hoeneisen 《International Journal of Astronomy and Astrophysics》 2017年第1期11-27,共17页
We measure the baryon acoustic oscillation (BAO) observables , , and as a function of red shift z in the range 0.1 to 0.7 with Sloan Digital Sky Survey (SDSS) data release DR13. These observables are independent and s... We measure the baryon acoustic oscillation (BAO) observables , , and as a function of red shift z in the range 0.1 to 0.7 with Sloan Digital Sky Survey (SDSS) data release DR13. These observables are independent and satisfy a consistency relation that provides discrimination against miss-fits due to background fluctuations. From these measurements and the correlation angle of fluctuations of the Cosmic Microwave Background (CMB), we obtain , and for dark energy density allowed to vary as . We present measurements of at six values of the expansion parameter a. Fits with several scenarios and data sets are presented. The data is consistent with space curvature parameter? and constant. 展开更多
关键词 Cosmology Dark Energy baryon Acoustic OSCILLATIONS
下载PDF
Constraints on Neutrino Masses from Baryon Acoustic Oscillation Measurements
11
作者 B. Hoeneisen 《International Journal of Astronomy and Astrophysics》 2018年第1期1-5,共5页
From 21 independent Baryon Acoustic Oscillation (BAO) measurements we obtain the following sum of masses of active Dirac or Majorana neutrinos: , where and . This result may be combined with independent measurements t... From 21 independent Baryon Acoustic Oscillation (BAO) measurements we obtain the following sum of masses of active Dirac or Majorana neutrinos: , where and . This result may be combined with independent measurements that constrain the parameters &Sigma;mv, h, and &Omega;bh2 . For?? and , we obtain at 95% confidence. 展开更多
关键词 NEUTRINO Mass baryon Accoustic OSCILLATIONS COSMOLOGY
下载PDF
Galaxy Evolution by the Incompatibility between Dark Matter and Baryonic Matter
12
作者 Ding-Yu Chung 《International Journal of Astronomy and Astrophysics》 2014年第2期374-383,共10页
The paper derives the galaxy evolution by the non-interacting (incompatibility) between dark matter and baryonic matter in terms of the short-range separation between dark matter and baryonic matter, so dark matter ca... The paper derives the galaxy evolution by the non-interacting (incompatibility) between dark matter and baryonic matter in terms of the short-range separation between dark matter and baryonic matter, so dark matter cannot contact baryonic matter. In the conventional CDM (cold dark matter) model, dark matter and baryonic matter are interactive (compatible), so dark matter can contact baryonic matter. However, the conventional CDM model fails to account for the failure to detect dark matter by the contact (interaction) between dark matter and baryonic matter, the shortage of small galaxies, the abundance of spiral galaxies, the old age of large galaxies, and the formation of thin spiral galaxies. The non-interacting (incompatible cold dark matter) model can account for these observed phenomena. The five periods of baryonic structure development in the order of increasing non-interacting (incompatibility) are the free baryonic matter, the baryonic droplet, the galaxy, the cluster, and the supercluster periods. 展开更多
关键词 GALAXY Evolution CDM DARK MATTER MOND baryonic MATTER INCOMPATIBLE DARK MATTER ICDM
下载PDF
Predicting the Neutron and Proton Masses Based on Baryons which Are Yang-Mills Magnetic Monopoles and Koide Mass Triplets
13
作者 Jay R. Yablon 《Journal of Modern Physics》 2013年第4期127-150,共24页
We show how the Koide relationships and associated triplet mass matrices can be generalized to derive the observed sum of the free neutron and proton rest masses in terms of the up and down current quark masses and th... We show how the Koide relationships and associated triplet mass matrices can be generalized to derive the observed sum of the free neutron and proton rest masses in terms of the up and down current quark masses and the Fermi vev to six parts in 10,000. This sum can then be solved for the separate neutron and proton masses using the neutron minus proton mass difference derived by the author in a recent, separate paper. The oppositely-signed charges of the up and down quarks are responsible for the appearance of a complex phase exp(iδ) and real rotation angle θ which leads on an independent basis to mass and mixing matrices similar to that of Cabibbo, Kobayashi and Maskawa (CKM). These can then be used to specify the neutron and proton mass relationships to unlimited accuracy using θ as a nucleon fitting angle deduced from empirical data. This fitting angle is then shown to be related to an invariant of the CKM mixing angles within experimental errors. Also developed is a master mass and mixing matrix which may help to interconnect all baryon and quark masses and mixing angles. The Koide generalizations developed here enable these neutron and proton mass relationships to be given a Lagrangian formulation based on neutron and proton field strength tensors that contain vacuum-amplified and current quark wavefunctions and masses. In the course of development, we also uncover new Koide relationships for the neutrinos, the up quarks, and the down quarks. 展开更多
关键词 PROTON MASS NEUTRON MASS baryonS Magnetic MONOPOLES Koide CKM Mixing Angles Current QUARKS Constituent QUARKS
下载PDF
Grand Unified SU(8) Gauge Theory Based on Baryons which Are Yang-Mills Magnetic Monopoles
14
作者 Jay R. Yablon 《Journal of Modern Physics》 2013年第4期94-120,共27页
Based on the thesis that baryons including protons and neutrons are Yang-Mills magnetic monopoles which the author has previously developed and which has been confirmed by over half a dozen empirically-accurate predic... Based on the thesis that baryons including protons and neutrons are Yang-Mills magnetic monopoles which the author has previously developed and which has been confirmed by over half a dozen empirically-accurate predictions, we develop a GUT that is rooted in the SU(4) subgroups for the proton/electron and neutron/neutrino which were used as the basis for these predictions. The SU(8) GUT group so-developed leads following three stages of symmetry breaking to all known phenomenology including a neutrino that behaves differently from other fermions, lepto-quark separation, replication of fermions into exactly three generations, the Cabibbo mixing of those generations, weak interactions which are left-chiral, and all four of the gravitational, strong, weak, and electromagnetic interactions. The next steps based on this development will be to calculate the masses and energies associated with the vacuum terms of the Lagrangian, to see if additional empirical confirmations can be achieved, especially for the proton and neutron and the fermion masses. 展开更多
关键词 GUT SU(8) YANG-MILLS baryonS Magnetic MONOPOLES Nuclear Physics Binding Energy Protons Neutrons Fermions QUARKS Electrons Neutrinos LEPTONS Generations Cabibbo Mixing Chirality Gravitation QCD ELECTROWEAK
下载PDF
A Unifying Theory of Dark Energy, Dark Matter, and Baryonic Matter in the Positive-Negative Mass Universe Pair: Protogalaxy and Galaxy Evolutions
15
作者 Ding-Yu Chung 《Journal of Modern Physics》 2020年第7期1091-1122,共32页
This paper modifies the Farnes’ unifying theory of dark energy and dark matter which are negative-mass, created continuously from the negative-mass universe in the positive-negative mass universe pair. The first modi... This paper modifies the Farnes’ unifying theory of dark energy and dark matter which are negative-mass, created continuously from the negative-mass universe in the positive-negative mass universe pair. The first modification explains that observed dark energy is 68.6%, greater than 50% for the symmetrical positive-negative mass universe pair. This paper starts with the proposed positive-negative-mass 11D universe pair (without kinetic energy) which is transformed into the positive-negative mass 10D universe pair and the external dual gravities as in the Randall-Sundrum model, resulting in the four equal and separate universes consisting of the positive-mass 10D universe, the positive-mass massive external gravity, the negative-mass 10D universe and the negative-mass massive external gravity. The positive-mass 10D universe is transformed into 4D universe (home universe) with kinetic energy through the inflation and the Big Bang to create positive-mass dark matter which is five times of positive-mass baryonic matter. The other three universes without kinetic energy oscillate between 10D and 10D through 4D, resulting in the hidden universes when D > 4 and dark energy when D = 4, which is created continuously to our 4D home universe with the maximum dark energy = 3/4 = 75%. In the second modification to explain dark matter in the CMB, dark matter initially is not repulsive. The condensed baryonic gas at the critical surface density induces dark matter repulsive force to transform dark matter in the region into repulsive dark matter repulsing one another. The calculated percentages of dark energy, dark matter, and baryonic matter are 68.6 (as an input from the observation), 26 and 5.2, respectively, in agreement with observed 68.6, 26.5 and 4.9, respectively, and dark energy started in 4.33 billion years ago in agreement with the observed 4.71 <span style="white-space:nowrap;">&plusmn;</span> 0.98 billion years ago. In conclusion, the modified Farnes’ unifying theory reinterprets the Farnes’ equations, and is a unifying theory of dark energy, dark matter, and baryonic matter in the positive-negative mass universe pair. The unifying theory explains protogalaxy and galaxy evolutions in agreement with the observations. 展开更多
关键词 Unifying Theory Farnes Dark Energy Dark Matter baryonic Matter Negative Mass Positive-Negative Mass Universe Pair Protogalaxy Evolution Galaxy Evolution
下载PDF
Electric Charge, Matter Distribution, and Baryon Asymmetry from Holographic Principle
16
作者 T. R. Mongan 《Journal of Modern Physics》 2021年第3期295-299,共5页
Explaining baryon asymmetry (<em>i.e.</em>, matter dominance) in the universe has been a vexing problem in physics. This analysis, based on the holographic principle, identifies fractional electric charge ... Explaining baryon asymmetry (<em>i.e.</em>, matter dominance) in the universe has been a vexing problem in physics. This analysis, based on the holographic principle, identifies fractional electric charge with the state of bits of information on the event horizon. Thermodynamics on the event horizon at the time of baryogenesis then estimates observed baryon asymmetry. 展开更多
关键词 Electric Charge baryon Asymmetry Holographic Principle
下载PDF
1-22 Baryon and Chiral Symmetry Breaking in Holographic QCD
17
作者 Sven Bjarke Gudnason 《IMP & HIRFL Annual Report》 2015年第1期33-33,共1页
We study the relationship between chiral symmetry breaking and baryons in holographic QCD. We construct a soliton with unit baryon charge in the presence of a nonzero mean value of the scalar bifundamental field, whic... We study the relationship between chiral symmetry breaking and baryons in holographic QCD. We construct a soliton with unit baryon charge in the presence of a nonzero mean value of the scalar bifundamental field, which is dual to the chiral condensate. We obtain a relation between the chiral condensate and the mass of the baryon, and find in a clear-cut way that at large values of the condensate, the holographic soliton is no longer located on the IR wall, being split into two halves, which are symmetrically located on the left and right flavor branes. On the other hand, we find that the local value of the quark condensate is suppressed in the core of the soliton, which is evidence for a partial chiral symmetry restoration inside the baryon. 展开更多
关键词 baryon CHIRAL SYMMETRY
下载PDF
Evidence for Non-Baryonic Dark Matter
18
作者 Matsuo Sekine 《Journal of High Energy Physics, Gravitation and Cosmology》 CAS 2022年第3期800-809,共10页
There exists an infinite number of quarks u(∞) and anti-quarks  at an infinite sub-layer level. These particles are considered as the ultimate building blocks of the universe, since they are structure-less and a... There exists an infinite number of quarks u(∞) and anti-quarks  at an infinite sub-layer level. These particles are considered as the ultimate building blocks of the universe, since they are structure-less and absolutely stable. These particles are also regarded as the non-baryonic dark matter, since the baryon number is zero and the R<sub>p</sub>-parity is -1. It is emphasized that supersymmetric particle, neutralino has also the R<sub>p</sub>-parity of -1 and well known good cold dark matter candidate. In modern particle physics, all ordinary particles have the R<sub>p</sub>-parity of +1, while both the ultimate quark u(∞) and neutralino have the R<sub>p</sub>-parity of -1. This means that these particles can only be created or annihilated in pairs in reactions of ordinary particles. From electron-positron annihilation experiments at high energies, it is shown that the prediction value from the ultimate quark u(∞) is in good agreement with many ring-storage collider experiments. 展开更多
关键词 Non-baryonic Dark Matter Negative Rp-Parity NEUTRALINO Electon-Positron Experiment
下载PDF
Breaking SU(3)Symmetry and Baryon Masses
19
作者 Kai-Wai Wong Gisela A.M.Dreschhoff Hogne J.N.Jungner 《Journal of Modern Physics》 2015年第11期1492-1497,共6页
Following the Projection-Gell-Mann Standard Model obtained from 5D homogeneous space-time, we extended to the definition of Strange and Charm quarks from the SU(3) fractional charged generators superposition represent... Following the Projection-Gell-Mann Standard Model obtained from 5D homogeneous space-time, we extended to the definition of Strange and Charm quarks from the SU(3) fractional charged generators superposition representations, and calculated all the well-known baryon masses. The results indicate how the Orthogonality between the SU(2) × L and SU(3) × L manifolds is broken in the hadrons, such that the superposition of the time projection Po, and the conformal space projection P1 are established, the basic requirement for General Relativity and the establishment of the Riemannian curvature in the presence of mass. 展开更多
关键词 GLUON SU(3)Breaking baryon Masses
下载PDF
A Simple Physical Approach to Study Spectrum of Baryons
20
作者 H.Hassanabadi 《Communications in Theoretical Physics》 SCIE CAS CSCD 2011年第2期303-306,共4页
The exact solution of Schrodinger equation corresponding to a baryonic system is the main interest in the present work.We take into account both quadratic and Coulomb terms in the potential relation.Next,after present... The exact solution of Schrodinger equation corresponding to a baryonic system is the main interest in the present work.We take into account both quadratic and Coulomb terms in the potential relation.Next,after presenting an exact solution,we have calculated the spin and isospin effects in both ground and excited states.The results are comparabJe with experimental data. 展开更多
关键词 重子谱 物理方法 同位旋效应 实验数据 精确解 激发态 可比性 方程
下载PDF
上一页 1 2 16 下一页 到第
使用帮助 返回顶部