A unified model with a generalized gauge symmetry and its cosmological implications

被引:4
作者
Hsu, Jong-Ping [1 ]
Cottrell, Kazuo O. [1 ]
机构
[1] Univ Massachusetts Dartmouth, Dept Phys, N Dartmouth, MA 02747 USA
关键词
unified model; nonintegrable phase factors; conservation laws; cosmology; accelerated expansion; YANG-MILLS GRAVITY; WEAK INTERACTIONS; ENERGY;
D O I
10.1088/1674-1137/39/10/105101
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
A unified model is based on a generalized gauge symmetry with groups [SU3c](color)x(SU(2)xU(1))x[U(1b)xU(11)]. It implies that all interactions should preserve conservation laws of baryon number, lepton number, and electric charge, etc. The baryonic U-1b, leptonic U-11 and color SU3c gauge transformations are generalized to involve nonintegrable phase factors. One has gauge invariant fourth-order equations for massless gauge fields, which leads to linear potentials in the [U-1b x U-11] and color [SU3c] sectors. We discuss possible cosmological implications of the new baryonic gauge field. It can produce a very small constant repulsive force between two baryon galaxies (or between two anti-baryon galaxies), where the baryon force can overcome the gravitational force at very large distances and leads to an accelerated cosmic expansion. Based on conservation laws in the unified model, we discuss a simple rotating dumbbell universe with equal amounts of matter and anti-matter, which may be pictured as two gigantic rotating clusters of galaxies. Within the gigantic baryonic cluster, a galaxy will have an approximately linearly accelerated expansion due to the effective force of constant density of all baryonic matter. The same expansion happens in the gigantic anti-baryonic cluster. Physical implications of the generalized gauge symmetry on charmonium confining potentials due to new SU3c field equations, frequency shift of distant supernovae Ia and their experimental tests are discussed.
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页数:9
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共 33 条
[1]   No-ghost theorem for the fourth-order derivative pais-uhlenbeck oscillator model [J].
Bender, Carl M. ;
Mannheim, Philip D. .
PHYSICAL REVIEW LETTERS, 2008, 100 (11)
[2]   Calculation of the hidden symmetry operator for a PT-symmetric square well [J].
Bender, CM ;
Tan, B .
JOURNAL OF PHYSICS A-MATHEMATICAL AND GENERAL, 2006, 39 (08) :1945-1953
[3]  
Bopp F, 1940, ANN PHYS-BERLIN, V38, P345
[4]   CP violation, fermion masses and mixings in a predictive SUSY SO(10)x Delta (48)xU(1) model with small tan beta [J].
Chou, KC ;
Wu, YL .
PHYSICAL REVIEW D, 1996, 53 (07) :R3492-R3495
[5]  
De Wet J.S, 1948, MATH PROC CAMBRIDGE, V44, P546
[6]  
Dyson F.J., 2005, 100 YEARS GRAVITY AC, P348
[7]   SPECTRUM OF CHARMED QUARK-ANTIQUARK BOUND-STATES [J].
EICHTEN, E ;
GOTTFRIED, K ;
KINOSHITA, T ;
KOGUT, J ;
LANE, KD ;
YAN, TM .
PHYSICAL REVIEW LETTERS, 1975, 34 (06) :369-372
[8]   ON A SYMMETRY IN WEAK INTERACTIONS [J].
GAMBA, A ;
MARSHAK, RE ;
OKUBO, S .
PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 1959, 45 (06) :881-885
[9]  
Hsu J P, 2013, SPACE TIME SYMMETRY, p[212, 225]
[10]   Yang-Mills gravity in flat space-time I: Classical gravity with translation gauge symmetry [J].
Hsu, Jong-Ping .
INTERNATIONAL JOURNAL OF MODERN PHYSICS A, 2006, 21 (25) :5119-5139