PROGRAM of the 23rd International workshop ‘’What comes beyond the standard models’’ [ Virtual Workshop ]
Program for Thursday, 9th of July 2020
Morning session:
Chair person: Dmitri Semikoz
9.00 - 10.00. Vitaly Beylin, On the reactions involving neutrinos and hidden mass particles in hypercolor model
The following questions and comments were made during this talk
Holger: What if any is the quantum number conservation that keeps you dark matter particles stable?
Holger: Why do your cross sections go down to zero for high energy of say your proton?
Holger: Yes differential cross section is not like total cross section
Norma: You have two three families = the ordinary and the additional-dark.
Norma: You have two three families = the ordinary and the additional-dark.
Norma: They distinguish in Higgses, while the colour, weak and U(1) is the same.
Norma: The dark matter is not very massive, at least not the last one
Holger: These arguments for looking for neutrinos would be valid almost whatever your dark matter model might be.
Norma: But they have to interact through what?
Norma: You need that they interact and they interact through electroweak
Norma: Your dark particles get masses through their own Higgses -sigmas?
Norma: How many parameter so you need?
10.00 – 11.00. Vladimir Kuksa, Main properties of new heavy hadrons and the luminosity of hadronic dark matter
The following questions and comments were made
Norma: You have Q_s, U,D Is Q left and right?
Holger: Remind us what is ZE effect
Norma: Mistake: I meant two right two right
Holger: Would so strong interactions keep the dark matter sufficiently dark to cope with the gravitational force knowledge about the distribution of DM in galaxy ?
Konstantin B.: This is a comment: I would like also to pay attention to our work
https://arxiv.org/abs/1909.04735 , where some constraints imposed from large scale structure (Fig.12, Eq.18 there).
Holger: What was your limits to your model from the non observation so far in sat LUX experiment
11:00 – 13:30. Antonino Marciano, Gravitational footprints of massive neutrinos and lepton number breaking
The following questions were put and comment made
Holger: How strongly can you find neutron stars vibrating ?
Holger: what means SKA?
Norma: Antonino, I shall be glad if you go through my spin-charge-family theory, which offers not only the explanation for the standard model s physics (HEP and cosmology) but offers also new fields and particles (dark matter, matter-antimatter asymmetry,..)
Holger 2: What is the symbol for the Majoron here?
Andrea Addazi: sigma
Afternoon session
Chair person: Antonino Marciano
15:00 – 16:30: Ulrich Jentschura, Lorentz Violation in the Neutrino Sector: New Stringent Contraints due to Additional Decay Channels Squeeze the Parameter Space.
The following question was put during this talk:
Holger: Is there similar but less stringent limits for other Lorentz breaking attempts?
16:30 –17:00: Albino Hernandez-Galeana, Neutrino masses and mixing within a SU(3) family symmetry model with sterile neutrinos. Part 2
17:00 – 18:30. Discussion of family problem (Norma Mankoc Bostnik, Albino Hernandez-Galeana, …)
Norma presented her explanation for the origin of families.
The following questions and comments were put:
Holger: How much do you improve you fit relative to the hypothesis that there are only three families and all mixing to the fourth thus zero?
Albino Hernandez: what about neutrinos in your approach?
Holger: So then you lost the in Standard Model natural way of glint light left neutrinos
21:00- 22.00 Preparation of program with discussions