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Figure 01 See-saw Mechanism |
HR + R
H
L) ---------- (1),
" denotes
= (L
)ij = (L*)ji.
0
Lmass
0.
,
,
). Such mixing in flight can happen only when the neutrinos have mass (see "Detection of Neutrino Mass").![]() |
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Figure 02 Neutrino Mass |
Figure 02 shows the estimated mass of the neutrinos ~ 106 - 1012 times smaller than the other fermions. |
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For m ~ 105 ev (~ mass of the electron), and M ~ 102 Gev (~ electro-weak symmetry breaking scale, see Figure 03), the neutrino mass would be of the order 0.1 ev. There is no need to reduce the strength for the Higgs coupling in this scenario. But the conservation of lepton number is violated. Such non-conserving process is still awaiting further experimental result (e.g., the neutrinoless double-beta-decay) to confirm. Although the seesaw model is extremely appealing in the sense that it gives a natural qualitative explanation of the smallness of neutrino masses, it still leaves too many possible reasonable combinations to use it for quantitative goals. |
Figure 03 Symmetry Breakings |
To recap : |
HR + R
H
L).
(m/M)L, where m is the Dirac mass, and M is actually just a parameter but considered to be the mass of the Majorana neutrino.
Ge(m/M)L
HL.
Gev(m/M)L
L.
L = 1,
LMajo
m2/M. ![]() |
baryogenesis) suggests that an exceptionally heavy but unstable breed of Majorana neutrino existed in the very early universe. Their subsequent decay generated more anti-leptons than leptons. A mechanism called "Sphaleron" then converted 1/3 of the excess anti-leptons into baryons leading to the imbalance between matter and antimatter at the dawn of time. Theoretical analysis shows that leptogenesis works best when the neutrino masses are in the range 0.1 ev - 1 mev; the mass of the Majorana neutrino and the reheating temperature must be larger than 109 Gev. |
Figure 04 Leptogenesis |
Such theory is the most favored mechanism to explain the matter anti-matter asymmetry because there is good circumstantial evidence for existence of various ingredients (except the requirement of heavy Majorana neutrino at reheating when particles were massless according to SM). See detail : |
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Figure 05 Leptogenesis, |
is similar to the last term of L3 with R (the right-handed lepton field) replaced by N (the right-handed heavy neutrino field) :![]() |
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Figure 06 Speed of Massless and Massive Particle [view large image] |
(see Figure 06). The Lagrangian above is for generating the so-called "Dirac mass". There is another mass producing mechanism by Majorana neutrino, which is its own anti-self (see "See-Saw"). |
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Figure 07 Lepton Lagrangian [view large image] |
This condition determines the time when equilibrium is reached in relation to the processing of the following differential equations. The rate of cosmic expansion slows down over time, i.e., non-equilibrium previals mostly at earlier time. |

~ 1012 sec-1 similar to many present-day meson decay.![]() |
where R is the scale factor for measuring the relative scale of the universe (R = 1, for the current epoch). The formula is : H = (8 G /3)1/2 ~ 2.4x1012 sec-1 (for t ~ 10-12 sec),where ~ 1031 gm/cm3 (Figure 08) even through particles are restmass-less ( m0 = 0) before SSB/ESB, this data is still meaningful since E = m0c2/[1-(v/c)2]1/2,
and the gravitational constant G = 6.67x10-8 cm3/sec2-gm. Thus, the wash-out indicator k ~ 0.4 indicating that the system is in non-equilibrium state around the time frame of 10-12 sec. |
Figure 08 Cosmic History |
E
t
= 10-27 erg-sec, if the N neutrino were created soon after the epoch of
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Inflation at 10-33 sec (see Figure 09), then its mass M (in term of energy E) should not be lower than /10-33, i.e., M 106 erg = 0.6x109 Gev. Similar argument can also be applied to its decay product of anti-neutrino produced up to 10-12 sec around the SSB/ESB transition givingMB-L 0.6x10-3 ev (most probably ~ 0.1 ev), which is compatible with experimental measurement. This is used as evidence to support the leptogensis theory.
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Figure 09 Early Universe |
.
= matter/radiation = 6x10-10. The present-day radiation number density = 411 cm-3 is interpreted as the result of matter/anti-matter annihilation leaving behind the baryonic number density ~ 2.5x10-7 cm-3.
= (1/3)(nB-L/411) which yields nB-L =
n0 = 7.5x10-7 cm-3.
n0 = 7.5x1068 cm-3, and the radiation number density is 411x1075 cm-3.
0 = 1054 gm/cm3.
0 = 1065 gm/cm3 at that time, thus
= 10-11 is required to account for the observed asymmetry by leptogenesis. The "B Meson Decay" experiments produce
~ 10-19 revealing that such CP violation mechanism is not sufficient. ![]() |
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However, this kind of source seems to be unlikely since UHECRs are isotropic, and not affected by magnetic fields. The yellow line in Figure 10 is the observed cosmic ray energy spectrum. The three other lines show how suspected sources possibly contribute to the overall signature of cosmic rays. It is not known what causes the kinks at the "knee" and "ankle". Normally, cosmic rays bombard the Earth at a rate of about 1 particle/km2-sec. At ultra-high energies, above 1010 Gev, the rate falls to less than 1 particle/km2-year. |
Figure 10 C-Rays Spectrum |
Figure 11 Cosmic Rays, Origins of [view large image] |
Figure 11 lists some of the sources such as Supernovae for High-Energy (up to 106 Gev), Black-holes for Medium Energy (up to 109 Gev). The UHECR (up to 1011 Gev) is the one difficult to explain. The following is an attemp to link such events to the right handed neutrinos in the very early universe. |
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Figure 12 Cosmic History |
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Figure 13 Dark Matter Properties [view large image] |
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times that of the proton. Most of these electrically neutral particles would, like neutrino, go straight through Earth. On rare occasion, however, one might interact with an atom in the material they pass through. So far, the only claimed detection of a dark matter particle (by an Italian team in 2000) has been strongly disputed. One particularly interesting WIMP is the lightest supersymmetric particle (LSP) - the neutralino, which could be a Majorana fermion (a particle which is its own antiparticle) and thus has more chance to produce the electron-positron pair. Figure 14 shows the region excluded in the dark-matter-mass vs WIMP-Nucleon-Cross-Section |
Figure 14 Dark Matter Constraints |
(via gravitational interaction) by various observations in the past or in the future (if nothing shows up).Anyway, Supersymmetry is becoming irrelevant as none of the super-partners show up in experiments (as of 2021). |
has to be introduced (see Figure 15,a and more Axion details). It evolved in the very early cosmic history starting soon after the inflation period, gradually generates an effect to cancel out the CP violation, and eventually acquires a steady mass (Figure 15,b).![]() |
= /f = 2.155 for making the CP violation disappeared. Such low mass allows for long life (since there are no lighter particles to decay into). The number density Na ~ 14x106/cm3 would be in agreement with DM = 0.23, if ma = 10-4 ev. |
Figure 15 Axion |
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Figure 16 Wimpzilla |
This one seems to have all the ingredients for dark matter too. It is just something like the neutrino except with heavy mass to keep it from moving too fast and to allow for sufficient amount similar to observation. However, it would not be the type proposed in leptogeneses, for which the life time is about 10-12 sec. |
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Although the Standard Model has been very successful in accounting for all experimental phenomena, it is not expected to be the ultimate theory because of the many problems (including neutrino mass now) it leaves unanswered. These objections suggest that there may be deeper symmetries underlying the standard model, leading perhaps to the unification of the strong and electroweak interactions into a single "Grand Unified theory (GUT)" at the dawn of time (see Figure 17). Such scheme is indeed possible if the internal rotation group is further generalized to SO(10). BTW, the SU(5) scheme is dead because its prediction of proton decay fails to materialized after more than 20 years of futile searches. |
Figure 17 Cosmic Evolution [view large image] |
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, e)L and (u, d)L while t3 = 0 for the right handed sector. |
Figure 18 SO(10) Group in GUT |
)R is the odd-man/woman out in the model. It is there to provide a possible mechanism for the mass of the neutrinos (and more). As Y = t3 = Q = 0,
it does not involve in any of the interactions. It just sits in the corner - never been detected (smelling like dark matter or something long gone ?). |