Slides of the talk on Koide Formula. Video should be available at http://viavca.in2p3.fr/alejandro_rivero.html
or directly al flv
http://viavca.in2p3.fr/video/alejandro_rivero.flv
Non-interacting and interacting Graphene in a strong uniform magnetic fieldAnkurDas60
We study monolayer graphene in a uniform magnetic field in the absence and presence of interactions. In the non-interacting limit for p/q flux quanta per unit cell, the central two bands have 2q Dirac points in the Brillouin zone in the nearest-neighbor model. These touchings and their locations are guaranteed by chiral symmetry and the lattice symmetries of the honeycomb structure. If we add a staggered potential and a next nearest neighbor hopping we find their competition leads to a topological phase transition. We also study the stability of the Dirac touchings to one-body perturbations that explicitly lowers the symmetry.
In the interacting case, we study the phases in the strong magnetic field limit. We consider on-site Hubbard and nearest-neighbor Heisenberg interactions. In the continuum limit, the theory has been studied before [1]. It has been found that there are four competing phases namely, ferromagnetic, antiferromagnetic, charge density wave, and Kekulé distorted phases. We find phase diagrams for q=3,4,5,6,9,12 where some of the phases found in the continuum limit are co-existent in the lattice limit with some phases not present in the continuum limit.
[1] M. Kharitonov PRB 85, 155439 (2012)
*NSF DMR-1306897
NSF DMR-1611161
US-Israel BSF 2016130
Binping xiao superconducting surface impedance under radiofrequency fieldthinfilmsworkshop
Based on BCS theory with moving Cooper pairs, the electron states distribution at 0 K and the probability of electron occupation with finite temperature have been derived and applied to anomalous skin effect theory to obtain the surface impedance of a superconductor under radiofrequency (RF) field. We present the numerical results for Nb and compare these with representative RF field-dependent effective surface resistance measurements from a 1.5 GHz resonant structure.
Non-interacting and interacting Graphene in a strong uniform magnetic fieldAnkurDas60
We study monolayer graphene in a uniform magnetic field in the absence and presence of interactions. In the non-interacting limit for p/q flux quanta per unit cell, the central two bands have 2q Dirac points in the Brillouin zone in the nearest-neighbor model. These touchings and their locations are guaranteed by chiral symmetry and the lattice symmetries of the honeycomb structure. If we add a staggered potential and a next nearest neighbor hopping we find their competition leads to a topological phase transition. We also study the stability of the Dirac touchings to one-body perturbations that explicitly lowers the symmetry.
In the interacting case, we study the phases in the strong magnetic field limit. We consider on-site Hubbard and nearest-neighbor Heisenberg interactions. In the continuum limit, the theory has been studied before [1]. It has been found that there are four competing phases namely, ferromagnetic, antiferromagnetic, charge density wave, and Kekulé distorted phases. We find phase diagrams for q=3,4,5,6,9,12 where some of the phases found in the continuum limit are co-existent in the lattice limit with some phases not present in the continuum limit.
[1] M. Kharitonov PRB 85, 155439 (2012)
*NSF DMR-1306897
NSF DMR-1611161
US-Israel BSF 2016130
Binping xiao superconducting surface impedance under radiofrequency fieldthinfilmsworkshop
Based on BCS theory with moving Cooper pairs, the electron states distribution at 0 K and the probability of electron occupation with finite temperature have been derived and applied to anomalous skin effect theory to obtain the surface impedance of a superconductor under radiofrequency (RF) field. We present the numerical results for Nb and compare these with representative RF field-dependent effective surface resistance measurements from a 1.5 GHz resonant structure.
We study Koide equation sequentially in a chain of mass triplets. We notice at
least a not previously published triplet whose existence allows to
built a quark mass hierarchy from fixed yukawas for
top and up quarks. Also, the new triplets are used to build mass predictions either
descending from the experimental values or top and bottom, or ascending
from the original triplet of charged leptons.
On the existence properties of a rigid body algebraic integralsMagedHelal1
In this article, we consider kinematical considerations of a rigid body rotating around a
given fixed point in a Newtonian force field exerted by an attractive center with a rotating
couple about their principal axes of inertia. The kinematic equations and their well-known
three elementary integrals of the problem are introduced. The existence properties of the
algebraic integrals are considered. Besides, we search as a special case of the fourth algebraic
integral for the problem of the rigid body’s motion around a fixed point under the action of a
Newtonian force field with an orbiting couple. Lagrange’s case and Kovalevskaya’s one are
obtained. The large parameter is used for satisfying the existing conditions of the algebraic
integrals. The comparison between the obtained results and the previous ones is arising. The
numerical solutions of the regulating system of motion are obtained utilizing the fourth order
Runge-Kutta method and plotted in some figures to illustrate the positive impact of the
imposed forces and torques on the behavior of the body at any time.
UCSD NANO 266 Quantum Mechanical Modelling of Materials and Nanostructures is a graduate class that provides students with a highly practical introduction to the application of first principles quantum mechanical simulations to model, understand and predict the properties of materials and nano-structures. The syllabus includes: a brief introduction to quantum mechanics and the Hartree-Fock and density functional theory (DFT) formulations; practical simulation considerations such as convergence, selection of the appropriate functional and parameters; interpretation of the results from simulations, including the limits of accuracy of each method. Several lab sessions provide students with hands-on experience in the conduct of simulations. A key aspect of the course is in the use of programming to facilitate calculations and analysis.
We study Koide equation sequentially in a chain of mass triplets. We notice at
least a not previously published triplet whose existence allows to
built a quark mass hierarchy from fixed yukawas for
top and up quarks. Also, the new triplets are used to build mass predictions either
descending from the experimental values or top and bottom, or ascending
from the original triplet of charged leptons.
On the existence properties of a rigid body algebraic integralsMagedHelal1
In this article, we consider kinematical considerations of a rigid body rotating around a
given fixed point in a Newtonian force field exerted by an attractive center with a rotating
couple about their principal axes of inertia. The kinematic equations and their well-known
three elementary integrals of the problem are introduced. The existence properties of the
algebraic integrals are considered. Besides, we search as a special case of the fourth algebraic
integral for the problem of the rigid body’s motion around a fixed point under the action of a
Newtonian force field with an orbiting couple. Lagrange’s case and Kovalevskaya’s one are
obtained. The large parameter is used for satisfying the existing conditions of the algebraic
integrals. The comparison between the obtained results and the previous ones is arising. The
numerical solutions of the regulating system of motion are obtained utilizing the fourth order
Runge-Kutta method and plotted in some figures to illustrate the positive impact of the
imposed forces and torques on the behavior of the body at any time.
UCSD NANO 266 Quantum Mechanical Modelling of Materials and Nanostructures is a graduate class that provides students with a highly practical introduction to the application of first principles quantum mechanical simulations to model, understand and predict the properties of materials and nano-structures. The syllabus includes: a brief introduction to quantum mechanics and the Hartree-Fock and density functional theory (DFT) formulations; practical simulation considerations such as convergence, selection of the appropriate functional and parameters; interpretation of the results from simulations, including the limits of accuracy of each method. Several lab sessions provide students with hands-on experience in the conduct of simulations. A key aspect of the course is in the use of programming to facilitate calculations and analysis.
This article continues the study of concrete algebra-like structures in our polyadic approach, when the arities of all operations are initially taken as arbitrary, but the relations between them, the arity shapes, are to be found from some natural conditions. In this way, the associative algebras, coassociative coalgebras, bialgebras and Hopf algebras are defined and investigated. They have many unusual features in comparison with the binary case. For instance, both algebra and its underlying field can be zeroless and nonunital, the existence of the unit and counit is not obligatory, the dimension of the algebra can be not arbitrary, but "quantized"; the polyadic convolution product and bialgebra can be defined, when algebra and coalgebra have unequal arities, the polyadic version of the antipode, the querantipode, has different properties. As a possible application to the quantum group theory, we introduce the polyadic version of the braidings, almost co-commutativity, quasitriangularity and the equations for R-matrix (that can be treated as polyadic analog of the Yang-Baxter equation). Finally, we propose another concept of deformation which is governed not by the twist map, but by the medial map, only the latter is unique in the polyadic case. We present the corresponding braidings, almost co-mediality and M-matrix, for which the compatibility equations are found.
Time Evolution of Density Parameters for Matter and Dark Energy and their Int...IJASRD Journal
In the framework of Brans-Dicke (BD) theory, the first part of the present study determines the time dependence of BD parameter, energy density and Equation of State (EoS) parameter of the cosmic fluid in a universe expanding with acceleration, preceded by a phase of deceleration. For this purpose, a scale factor has been so chosen that the deceleration parameter, obtained from it, shows a signature flip with time. Considering the dark energy to be responsible for the entire pressure, the time evolution of energy parameters for matter and dark energy and the EoS parameter for dark energy have been determined. A model for an effective interaction term, between matter and dark energy, has been proposed and calculated. Its negative value at the present time indicates conversion of matter into dark energy. Using this term, the time dependence of the rates of change of matter and dark energy has been determined. It is found that the nature of dependence of the scalar field upon the scale factor plays a very important role in governing the time evolution of the cosmological quantities studied here. The present study provides us with a simple way to determine the time evolution of dark energy for a homogeneous and isotropic universe of zero spatial curvature, without involving any self-interaction potential or cosmological constant in the formulation.
Quantum-Gravity Thermodynamics, Incorporating the Theory of Exactly Soluble Active Stochastic Processes, with Applications
by Daley, K.
Published in IJTP in 2009. http://adsabs.harvard.edu/abs/2009IJTP..tmp...67D
Exact Solutions of Axially Symmetric Bianchi Type-I Cosmological Model in Lyr...IOSR Journals
In this paper we have obtained axially symmetric Bianchi type-I cosmological models for perfect
fluid distribution in the context of Lyra’s manifold. Exact solutions of the field equations are obtained by
assuming the expansion in the model is proportional to the shear . This leads to the condition
A Bn
where A and B are scale factors and n( 0) is a constant. Some kinematical and physical parameters of the
model have been discussed. The solutions are compatible with recent observations.
DERIVATION OF MODIFIED BERNOULLI EQUATION WITH VISCOUS EFFECTS AND TERMINAL V...Wasswaderrick3
In this book, we use conservation of energy techniques on a fluid element to derive the Modified Bernoulli equation of flow with viscous or friction effects. We derive the general equation of flow/ velocity and then from this we derive the Pouiselle flow equation, the transition flow equation and the turbulent flow equation. In the situations where there are no viscous effects , the equation reduces to the Bernoulli equation. From experimental results, we are able to include other terms in the Bernoulli equation. We also look at cases where pressure gradients exist. We use the Modified Bernoulli equation to derive equations of flow rate for pipes of different cross sectional areas connected together. We also extend our techniques of energy conservation to a sphere falling in a viscous medium under the effect of gravity. We demonstrate Stokes equation of terminal velocity and turbulent flow equation. We look at a way of calculating the time taken for a body to fall in a viscous medium. We also look at the general equation of terminal velocity.
This presentation explores a brief idea about the structural and functional attributes of nucleotides, the structure and function of genetic materials along with the impact of UV rays and pH upon them.
Salas, V. (2024) "John of St. Thomas (Poinsot) on the Science of Sacred Theol...Studia Poinsotiana
I Introduction
II Subalternation and Theology
III Theology and Dogmatic Declarations
IV The Mixed Principles of Theology
V Virtual Revelation: The Unity of Theology
VI Theology as a Natural Science
VII Theology’s Certitude
VIII Conclusion
Notes
Bibliography
All the contents are fully attributable to the author, Doctor Victor Salas. Should you wish to get this text republished, get in touch with the author or the editorial committee of the Studia Poinsotiana. Insofar as possible, we will be happy to broker your contact.
Comparing Evolved Extractive Text Summary Scores of Bidirectional Encoder Rep...University of Maribor
Slides from:
11th International Conference on Electrical, Electronics and Computer Engineering (IcETRAN), Niš, 3-6 June 2024
Track: Artificial Intelligence
https://www.etran.rs/2024/en/home-english/
Professional air quality monitoring systems provide immediate, on-site data for analysis, compliance, and decision-making.
Monitor common gases, weather parameters, particulates.
Richard's aventures in two entangled wonderlandsRichard Gill
Since the loophole-free Bell experiments of 2020 and the Nobel prizes in physics of 2022, critics of Bell's work have retreated to the fortress of super-determinism. Now, super-determinism is a derogatory word - it just means "determinism". Palmer, Hance and Hossenfelder argue that quantum mechanics and determinism are not incompatible, using a sophisticated mathematical construction based on a subtle thinning of allowed states and measurements in quantum mechanics, such that what is left appears to make Bell's argument fail, without altering the empirical predictions of quantum mechanics. I think however that it is a smoke screen, and the slogan "lost in math" comes to my mind. I will discuss some other recent disproofs of Bell's theorem using the language of causality based on causal graphs. Causal thinking is also central to law and justice. I will mention surprising connections to my work on serial killer nurse cases, in particular the Dutch case of Lucia de Berk and the current UK case of Lucy Letby.
What is greenhouse gasses and how many gasses are there to affect the Earth.moosaasad1975
What are greenhouse gasses how they affect the earth and its environment what is the future of the environment and earth how the weather and the climate effects.
Remote Sensing and Computational, Evolutionary, Supercomputing, and Intellige...University of Maribor
Slides from talk:
Aleš Zamuda: Remote Sensing and Computational, Evolutionary, Supercomputing, and Intelligent Systems.
11th International Conference on Electrical, Electronics and Computer Engineering (IcETRAN), Niš, 3-6 June 2024
Inter-Society Networking Panel GRSS/MTT-S/CIS Panel Session: Promoting Connection and Cooperation
https://www.etran.rs/2024/en/home-english/
Phenomics assisted breeding in crop improvementIshaGoswami9
As the population is increasing and will reach about 9 billion upto 2050. Also due to climate change, it is difficult to meet the food requirement of such a large population. Facing the challenges presented by resource shortages, climate
change, and increasing global population, crop yield and quality need to be improved in a sustainable way over the coming decades. Genetic improvement by breeding is the best way to increase crop productivity. With the rapid progression of functional
genomics, an increasing number of crop genomes have been sequenced and dozens of genes influencing key agronomic traits have been identified. However, current genome sequence information has not been adequately exploited for understanding
the complex characteristics of multiple gene, owing to a lack of crop phenotypic data. Efficient, automatic, and accurate technologies and platforms that can capture phenotypic data that can
be linked to genomics information for crop improvement at all growth stages have become as important as genotyping. Thus,
high-throughput phenotyping has become the major bottleneck restricting crop breeding. Plant phenomics has been defined as the high-throughput, accurate acquisition and analysis of multi-dimensional phenotypes
during crop growing stages at the organism level, including the cell, tissue, organ, individual plant, plot, and field levels. With the rapid development of novel sensors, imaging technology,
and analysis methods, numerous infrastructure platforms have been developed for phenotyping.
Toxic effects of heavy metals : Lead and Arsenicsanjana502982
Heavy metals are naturally occuring metallic chemical elements that have relatively high density, and are toxic at even low concentrations. All toxic metals are termed as heavy metals irrespective of their atomic mass and density, eg. arsenic, lead, mercury, cadmium, thallium, chromium, etc.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
2. nal
Koide formula: beyond charged leptons
The waterfall in the quark sector
Alejandro Rivero
Institute for Biocomputation and Physics of Complex Systems (BIFI)
Universidad de Zaragoza
October 3, 2014
arivero@unizar.es Koide Formula
4. nal
By Koide formula" we refer to a formula found by Y. Koide for charged
leptons, exact enough to predict tau mass within experimental limits
(me + m + m ) =
2
3
(
p
me +
p
m +
p
m )2
exp, in MeV: 1882:99 = 1882:97
It was found in the context of composite models of quarks and leptons,
but can be produced more generally.
More informally, we also call Koide formula to its generalisations and
look-alikes
other unexplained
7. nal
potential model
It is possible consider mi as a composite of two entities with charge Q0
and Qi such that
mi /
1
2
Q2
0 + Q0Qi +
1
2
Q2
i
and asking the matching conditions
P
Qi = 0 and
P
Q2
i =
P
Q2
0 .
From here it is clear that
p
m can have a negative sign sometimes.
The generalisation to more than three particles simply substitutes
3=2 by n=2. Of course, with more particles in the formula, the
probability of
8. nding a random coincidence increases.
arivero@unizar.es Koide Formula
10. nal
circle model
[MDS, Rosen 2007] suggested to use the notation
mk = M0
1 +
p
2 cos
2
3
k + 0
2
And particularly for charged leptons:
Me = 313:8MeV; e = 0:222
arivero@unizar.es Koide Formula
12. nal
Composites and Cabibbo angle
Later observations
Recent Work
F. Wilczek and A. Zee,
Discrete Flavor Symmetries and a Formula for the Cabibbo Angle,
Phys. Lett. B 70, 418 (1977) [Erratum-ibid. 72B, 504 (1978)].
tan c =
r
md
ms
H. Harari, H. Haut and J. Weyers,
Quark Masses And Cabibbo Angles,
Phys. Lett. B 78 (1978) 459.
mu = 0;
md
ms
=
2
p
3
2 +
p
3
While trivial, this is the
16. nal
Composites and Cabibbo angle
Later observations
Recent Work
Y. Koide,
A New Formula For The Cabibbo Angle And Composite Quarks And
Leptons,
Phys. Rev. Lett. 47 (1981) 1241.
Quark And Lepton Masses Speculated From A Subquark Model,
preprint (1981)
A Fermion - Boson Composite Model Of Quarks And Leptons,
Phys. Lett. B 120, 161 (1983).
A New View Of Quark And Lepton Mass Hierarchy,
Phys. Rev. D 28 (1983) 252.
In 1981, measured lepton mass was still 1783 4 MeV,
Koide simplest model predicted 1776:97
arivero@unizar.es Koide Formula
18. nal
Composites and Cabibbo angle
Later observations
Recent Work
Y. Koide
Should The Renewed Tau Mass Value 1777-Mev Be Taken Seriously?
Mod.Phys.Lett. A8 (1993) 2071
R. Foot,
A Note on Koide's lepton mass relation,
MCGILL-94-09 [arXiv:hep-ph/9402242]
p
m1;
(
p
m2;
p
m3)(1; 1; 1) = 45
S. Esposito and P. Santorelli,
A Geometric picture for fermion masses,
Mod. Phys. Lett. A 10, 3077 (1995) Considers quarks, family-wise, and
also neutrinos.
From 1995 to 2005 there is a gap
arivero@unizar.es Koide Formula
20. nal
Composites and Cabibbo angle
Later observations
Recent Work
N. Li and B. Q. Ma,
Estimate of neutrino masses from Koide's relation,
Phys. Lett. B 609, 309 (2005) (received 15 October 2004)
April 23 2005
I comment on Li and Ma paper, and older ones on Koide formula, online
at sci.physics.research and www.physicsforums.com. I am not the only
one who is astonished, and other papers will follow.
A. Rivero and A. Gsponer, [hep-ph/0505220]
The Strange formula of Dr. Koide,
Y. Koide, [hep-ph/0506247].
Challenge to the mystery of the charged lepton mass formula,
arivero@unizar.es Koide Formula
22. nal
Composites and Cabibbo angle
Later observations
Recent Work
J.-M. Gerard, F. Gonet and M. Herquet,
A New look at an old mass relation,
Phys. Lett. B 633, 563 (2006)
Sensibility to the renormalization group
Y Koide had already considered the sensibility to the running, but in early
2006 a pair of independent assessments are produced.
N. Li and B. Q. Ma,
Energy scale independence of Koide's relation for quark and lepton
masses,
Phys. Rev. D 73, 013009 (2006)
Z. z. Xing and H. Zhang,
On the Koide-like relations for the running masses of charged leptons,
neutrinos and quarks,
Phys. Lett. B 635, 107 (2006)
arivero@unizar.es Koide Formula
24. nal
Composites and Cabibbo angle
Later observations
Recent Work
C. A. Brannen, [preprint (2006)]
The Lepton Masses,
Alerts of the possibility of using negative signs in the formula and applies
it to neutrinos
G. Rosen,
Heuristic development of a Dirac-Goldhaber model for lepton and quark
structure,
Mod. Phys. Lett. A 22, 283 (2007).
Promotes the use of the formula as (313:85773MeV)
1 +
p
2 cos k
2
.
In this way, the question of the signs is automatically considered.
Curiously, nobody remarks that 313 MeV is the mass of a QCD quark.
As far as I know, this coincidence has not been useful for any model.
arivero@unizar.es Koide Formula
26. nal
Composites and Cabibbo angle
Later observations
Recent Work
F. Gonet,
A Bottom-up approach to fermion masses,
These Univ. Cath. de Louvain, (2008)
Proposes some generalisations, as well as a formula containing the
solutions to the equation jointly with spurious ones, so that the square
roots are not needed.
Y. Sumino,
Family Gauge Symmetry and Koide's Mass Formula,
Phys. Lett. B 671, 477 (2009)
Y. Sumino,
Family Gauge Symmetry as an Origin of Koide's Mass Formula and
Charged Lepton Spectrum,
JHEP 0905, 075 (2009)
arivero@unizar.es Koide Formula
28. nal
Composites and Cabibbo angle
Later observations
Recent Work
Y. Koide
Charged Lepton Mass Relations in a Supersymmetric Yukawaon Model
Phys. Rev. D 79, 033009 (2009)
M. D. Sheppeard, blog entries, (2010)
pseudomonad.blogspot.com.es/2010/11/theory-update-19.html
pseudomonad.blogspot.com.es/2010/07/m-theory-lesson-342.html
Notes that e = 3uct and dsb = 2uct
(see also [Zenczykowski 2012], who uses e = 3uct )
arivero@unizar.es Koide Formula
30. nal
Composites and Cabibbo angle
Later observations
Recent Work
W. Rodejohann and H. Zhang, [arXiv:1101.5525].
Extended Empirical Fermion Mass Relation,
Phys. Lett. B 698 (2011) 152
Only in the preprint version
Using PDG values, Pmt = 172:9, mb = 4:19, and mc = 1:29 GeV, 2 p
m=
P
m is about 1:495
A. Kartavtsev, arXiv:1111.0480
A remark on the Koide relation for quarks,
F. G. Cao,
Neutrino masses from lepton and quark mass relations...
Phys. Rev. D 85, 113003 (2012)
This is the
31. rst mention of the t; b; c tuple in the peer reviewed literature.
P. Zenczykowski,
Remark on Koide's Z3-symmetric parametrization of quark masses,
Phys. Rev. D 86, 117303 (2012)
arivero@unizar.es Koide Formula
33. nal
Year 2011
Beyond S3 symmetry
Koide Waterfall
Empirical waterfall
Solve for Koide and choose always the smaller solution
Solve et Itera
m3 =
(
p
m1 +
p
m2)
2
s
3 + 6
p
m1m2
p
m1 +
(
p
m2)2
!!2
mt mb mc ms mq mq0
. ( 173:21 ; 4:18 ) ! 1:3676
1346:84 ( 4:18 ; 1:3676 ) ! :09312
60:31 . ( 1:3676 ; :09312 ) ! :00003187
3558:3 34:72 . ( :09312 ; :00003187 ) ! :005441
1:996 1:227 :008156
pdg2014 : 1:275 :095 :0023 :0048
0:025 0:005 0:0006 0:0004
As expected, we get good predictions for the charm and strange quarks.
We could interpret q as the up quark, q0 as the down quark.
But the remarkable detail is that mq 0. We will use this fact later.
arivero@unizar.es Koide Formula
35. nal
Year 2011
Beyond S3 symmetry
Koide Waterfall
Are ther other tuples?
with a 1% of tolerance: (cbt) and (scb).
within a 10 % (usc), (dsb) and (dsc) can
36. t
considering Renormalization Group
For (s; c; b), the quotient LHS/RHS of Koide formula using running
masses from [XZ 2006] at MZ is 0.949, at GUT scale it is 0.947.
For GUT-level masses within a 10% of tolerance, we have still the
same triplets
arivero@unizar.es Koide Formula
38. nal
Year 2011
Beyond S3 symmetry
Koide Waterfall
Example
S4 is the group of permutations of the four diagonal axis of a cube. It is
the semidirect product of Klein Viergruppe times S3
S4 = V4 n S3
bds usc scb cbt
uct btd tdb dus
mixed families
2; brgb; e; urgb
; crgb; 3; drgb
; srgb; 1; trgb
Think SU(4) Pati-Salam with a
twist.
A similar rotation of the quarks was
suggested in [HHW78]
arivero@unizar.es Koide Formula
40. nal
Year 2011
Beyond S3 symmetry
Koide Waterfall
remember mq = 0?
If in some limit there is a massless particle, things are more predictive.
We can just
41. x the scale of the most massive element.
For four levels, the solution is
unique. We assume that the
massless particle is the up quark.
mb 4Mscb
m mc
p
3
2 Mscb
2+
m ms
p
3
2 Mscb
2
me mu 0
Mscb is 3Me
scb = 45, and e = 15
We can add an extra level above
and below and
42. x the scale telling
that the yukawa of the top is exactly
yt = 1
mt 174:1 GeV
mb 3:64 GeV
m mc 1:698 GeV
m ms 121:95 MeV
me mu 0 MeV
md 8:75 MeV
scb = 3e
In Foot's interpretation, e and scb would be orthogonal vectors
arivero@unizar.es Koide Formula
44. nal
Year 2011
Beyond S3 symmetry
Koide Waterfall
Climbing the Cascade
We take me and m as inputs, and the approximations detected in the
previous slide:
Mscb = 3Me
scb = 3e
exp:pdg14 pred:
t 173:21 0:087 173:26
b 4:18 0:03 4:197
c 1:275 0:025 1:359
1:77682(16) 1:776968
s 95 5 92:275
d 4:8 5:32
u 2:3 :0356
arivero@unizar.es Koide Formula
46. nal
Mesons
Other mass scales
tuples from heavy quark masses and the pion mass
Is QCD acting in Koide scene?
(0 +
p
M0 +
p
MD0 )2
0 + M0 + MD0
= 1:5017
(
p
M0 +
p
MD0 +
p
MB0 )2
M0 + MD0 + MB0
= 1:4923
Not bad, even if due to the coincidence (
47. ne-tuning?) ms M
We could add mesons and diquarks to our three-layer arrangement.
c bu; bc bs; bd B0;B0
s ; B
2; brgb; e; urgb B+;B+
0; B
0
s 5279:59MeV
s sc; dc bb; dd b; c ;D0;D0 1864:85MeV
; crgb; 3; drgb D+;D+
; srgb; 1; trgb +;K+ su; du ss; sd 8; 0;K0; K
0 134:9767MeV
Quark-Hadron Supersymmetry?
Same number of degrees of freedom.
arivero@unizar.es Koide Formula
49. nal
Mesons
Other mass scales
The Small Seesaw
Is electroweak GWS acting in Koide scene?
ln 2
s c
p
W Z0
t
u d
b
e v
103 102 101 100 101 102
12
g0
12
g0cos
12
g0sin
313:6 MeV
H0
GeV
From D. Lackey in a comment in [MDS]:
MZ sin W = 313:66 MeV.
(Using cos W = 0:8819) The relationship e is well
known, used in the early 70s. From to the electroweak vac-
uum, I read it
50. rst in a comment of R. Yablon in USENET.
arivero@unizar.es Koide Formula
52. nal
Mesons
Other mass scales
The Koide phase
Masses for 0 from 0 to 2=3, with M0 = 1;
0
12
7
12
4
3
2
3
3 + 2
p
2
p
2
3 2
4
1
arivero@unizar.es Koide Formula
54. nal
References
arXiv:hep-ph/0505220 A. Rivero, A. Gsponer
The strange formula of Dr. Koide
arXiv:1111.7232 A. Rivero
A new Koide tuple: strange-charm-bottom
Another presentacion online, with a lot of zooms:
http://prezi.com/e2hba7tkygvj/koide-waterfall/
contact
al.rivero@gmail.com arivero@unizar.es
Thank You!
arivero@unizar.es Koide Formula