Intermediate mass scale of SU(N) grand unification with nontrivial charge assignment

1985 ◽  
Vol 31 (11) ◽  
pp. 2964-2967
Author(s):  
Chung Ku Kim ◽  
Jae Kwan Kim
2006 ◽  
Vol 15 (06) ◽  
pp. 1175-1182
Author(s):  
V. ELIAS ◽  
T. G. STEELE

We demonstrate to two-loop order that an intermediate symmetrically embedded Pati–Salam SU(2)L×SU(2)R×SU(4) level of symmetry is all that is necessary to accommodate empirical values of α(Mz), αs(Mz) and sin 2θw(Mz) within a grand unification context but with a high (1014 GeV) intermediate mass scale and with a concomitant higher GUT scale.


1987 ◽  
Vol 02 (02) ◽  
pp. 133-143 ◽  
Author(s):  
F. FERUGLIO ◽  
F. GABBIANI

We build a realistic E6 superstring inspired model with intermediate mass scales, which has the characteristic feature of containing no extra U(1) factors in the low energy scenario. This may be acquired starting from a suitable Calabi-Yau compactification with b1.1>1, such to give rise, after Hosotani breaking, to the rank r=5 gauge group SU (3)C× SU (2)L×U(1)Y× U (1)E, that is broken at an intermediate mass scale down to the standard model group. The minimization of the low energy effective potential and the renormalization group analysis are quantitatively performed, yielding viable mass spectra.


1983 ◽  
Vol 70 (4) ◽  
pp. 1084-1090
Author(s):  
T. Watanabe ◽  
N. Toyota
Keyword(s):  

2021 ◽  
Vol 2021 (1) ◽  
Author(s):  
David J. E. Marsh ◽  
Wen Yin

Abstract An axion-like particle (ALP) with mass mϕ ∼ 10−15 eV oscillates with frequency ∼1 Hz. This mass scale lies in an open window of astrophysical constraints, and appears naturally as a consequence of grand unification (GUT) in string/M-theory. However, with a GUT-scale decay constant such an ALP overcloses the Universe, and cannot solve the strong CP problem. In this paper, we present a two axion model in which the 1 Hz ALP constitutes the entirety of the dark matter (DM) while the QCD axion solves the strong CP problem but contributes negligibly to the DM relic density. The mechanism to achieve the correct relic densities relies on low-scale inflation (mϕ ≲ Hinf ≲ 1 MeV), and we present explicit realisations of such a model. The scale in the axion potential leading to the 1 Hz axion generates a value for the strong CP phase which oscillates around $$ {\overline{\theta}}_{\mathrm{QCD}}\sim {10}^{-12} $$ θ ¯ QCD ∼ 10 − 12 , within reach of the proton storage ring electric dipole moment experiment. The 1 Hz axion is also in reach of near future laboratory and astrophysical searches.


1988 ◽  
Vol 60 (18) ◽  
pp. 1817-1820 ◽  
Author(s):  
R. Arnowitt ◽  
Pran Nath
Keyword(s):  

1979 ◽  
Vol 43 (12) ◽  
pp. 890-890 ◽  
Author(s):  
R. Brout ◽  
F. Englert ◽  
P. Spindel
Keyword(s):  

1979 ◽  
Vol 43 (6) ◽  
pp. 417-420 ◽  
Author(s):  
R. Brout ◽  
F. Englert ◽  
P. Spindel
Keyword(s):  

1983 ◽  
Vol 228 (2) ◽  
pp. 242-258 ◽  
Author(s):  
J. Maalampi ◽  
J. Pulido
Keyword(s):  

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