« Principe 7 » De La Pédagogie, Effet Zeeman-Effet Prérequis, Architecture Pyramidale Du Système Lmd: Mise En Œuvre D’une Pédagogie Discriminatoire Pour Un Enseignement De Qualité

In this work, we demonstrate by analogy with the quantified levels of atomic systems, that the levels of education from elementary to Superior are "quantified". The transition of a learner from one level of instruction to another is analogous to an electronic transition between atomic levels. The notions of ground state, excited states and ionized state of atomic systems have their equivalents in the school and university systems. It is demonstrated in this work that the number 7 is revealed in all countable elements of an educational system. This leads to the statement of the "principle 7 " of pedagogy. Thus, there are 7 levels of instruction or teaching-learning in the elementary, 7 levels at the middle-level and 7 levels of teaching-learning at the higher level. In addition, there are 7 degrees, 7 hours of work of the learner in the school space. The application of "Principle 7 of pedagogy" to the determination of the number of classes per cycle and the number of students per classroom is discussed. Moreover, it is shown in this work, that the Pauli Exclusion Principle allows to account for the correct occupation of the tablesbenches by the learners and that and the indiscernibility principle of the particles accounts for the necessity of the wearing school clothes. By analogy with the Zeeman Effect, it is shown that all levels of teaching-learning are degenerate. The lifting of degeneration by "Prerequisite Effect" highlights the need to put into practice a discriminatory pedagogy for quality education at the elementary level as well as at the higher level. Finally, it is demonstrated by analogy with the tightening of the atomic levels with the increase of the principal quantum number, that the architecture of the LDM must have the appearance of a pyramid, the base being constituted by the level License and the summit by the PhD level. Moreover, the increase in the number of 180/120/180 credits does not follow the pyramidal architecture of the LMD and that it should mathematically decrease according to the ratio L / M = M / D = 3/2; which corresponds to the 180/120/80 pyramidal progression. If a credit corresponds to 20 hours of work in L and M, it should correspond to 45 hours of work in D.

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Non-commutative quantum gravity phenomenology in underground experiments

Modern Physics Letters A ◽

10.1142/s0217732319502365 ◽

2019 ◽

Vol 34 (29) ◽

pp. 1950236 ◽

Cited By ~ 5

Author(s):

Andrea Addazi ◽

Rita Bernabei

Keyword(s):

Laboratory Experiments ◽

Planck Scale ◽

Pauli Exclusion Principle ◽

Energy Scale ◽

Exclusion Principle ◽

Atomic Systems ◽

Quantum Gravity Phenomenology ◽

Nuclear Transitions ◽

Moyal Plane ◽

Very High

We show how non-commutative spacetime models can induce Pauli Exclusion Principle (PEP) forbidden nuclear and atomic transitions. We focalize our analysis on one of the most popular instantiations of non-commutativeness: [Formula: see text]-Poincaré model, based on the Groenewold–Moyal plane algebra. We show that PEP violating transitions induced by [Formula: see text]-Poincaré have an energy scale and angular emission dependence. PEP violating transitions in nuclear and atomic systems can be tested with very high accuracy in underground laboratory experiments such as DAMA/LIBRA and VIP(2). We derive that the Equivalence Principle assumed [Formula: see text]-Poincaré model can be already ruled-out until the Planck scale, from nuclear transitions tests by DAMA/LIBRA experiment.

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Tests of Pauli exclusion principle violations from noncommutative quantum gravity

International Journal of Modern Physics A ◽

10.1142/s0217751x20420014 ◽

2020 ◽

Vol 35 (32) ◽

pp. 2042001

Author(s):

Andrea Addazi ◽

Rita Bernabei

Keyword(s):

Planck Scale ◽

Pauli Exclusion Principle ◽

Space Time ◽

Exclusion Principle ◽

Noncommutative Space ◽

Atomic Systems ◽

Nuclear Transitions ◽

Moyal Plane ◽

Spin Statistic ◽

Very High

We review the main recent progresses in noncommutative space–time phenomenology in underground experiments. A popular model of noncommutative space–time is [Formula: see text]-Poincaré model, based on the Groenewold–Moyal plane algebra. This model predicts a violation of the spin-statistic theorem, in turn implying an energy and angular dependent violation of the Pauli exclusion principle. Pauli exclusion principle violating transitions in nuclear and atomic systems can be tested with very high accuracy in underground laboratory experiments such as DAMA/LIBRA and VIP(2). In this paper we derive that the [Formula: see text]-Poincaré model can be already ruled-out until the Planck scale, from nuclear transitions tests by DAMA/LIBRA experiment.

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Modeling of electromagnetic waves propagation in four-level two-electron atomic systems governed by Pauli Exclusion Principle using the TLM method

Journal of Microwaves Optoelectronics and Electromagnetic Applications ◽

10.1590/s2179-10742012000100010 ◽

2012 ◽

Vol 11 (1) ◽

pp. 122-129

Author(s):

H. El Faylali ◽

M. Iben Yaich ◽

M. Khalladi ◽

A. Rafaoui

Keyword(s):

Electromagnetic Waves ◽

Pauli Exclusion Principle ◽

Exclusion Principle ◽

Atomic Systems ◽

Tlm Method ◽

Waves Propagation

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Hardness and HOMO-LUMO Gap Probed by the Helium Atom Pushing the Molecular Surface of the First-Row Hydride Molecules

Collection of Czechoslovak Chemical Communications ◽

10.1135/cccc20032344 ◽

2003 ◽

Vol 68 (12) ◽

pp. 2344-2354 ◽

Cited By ~ 3

Author(s):

Edyta Małolepsza ◽

Lucjan Piela

Keyword(s):

Helium Atom ◽

Pauli Exclusion Principle ◽

Structure Change ◽

Molecular Surface ◽

Exclusion Principle ◽

Probe Position ◽

Repulsion Energy ◽

Ionic Dissociation ◽

Probe Site ◽

Homo Lumo

A molecular surface defined as an isosurface of the valence repulsion energy may be hard or soft with respect to probe penetration. As a probe, the helium atom has been chosen. In addition, the Pauli exclusion principle makes the electronic structure change when the probe pushes the molecule (at a fixed positions of its nuclei). This results in a HOMO-LUMO gap dependence on the probe site on the isosurface. A smaller gap at a given probe position reflects a larger reactivity of the site with respect to the ionic dissociation.

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Identical Particles and Second Quantization: Occupation Number Representation

10.1093/oso/9780198791942.003.0002 ◽

2018 ◽

Author(s):

Norman J. Morgenstern Horing

Keyword(s):

Occupation Number ◽

Annihilation Operator ◽

Pauli Exclusion Principle ◽

Exclusion Principle ◽

Number Representation ◽

Second Quantization ◽

Identical Particles ◽

Fundamental Properties ◽

Minimum Uncertainty ◽

Creation Operators

Focusing on systems of many identical particles, Chapter 2 introduces appropriate operators to describe their properties in terms of Schwinger’s “measurement symbols.” The latter are then factorized into “creation” and “annihilation” operators, whose fundamental properties and commutation/anticommutation relations are derived in conjunction with the Pauli exclusion principle. This leads to “second quantization” with the Hamiltonian, number, linear and angular momentum operators expressed in terms of the annihilation and creation operators, as well as the occupation number representation. Finally, the concept of coherent states, as eigenstates of the annihilation operator, having minimum uncertainty, is introduced and discussed in detail.

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Testing the Pauli Exclusion Principle for Electrons at LNGS

Physics Procedia ◽

10.1016/j.phpro.2014.12.002 ◽

2015 ◽

Vol 61 ◽

pp. 552-559 ◽

Cited By ~ 2

Author(s):

H. Shi ◽

S. Bartalucci ◽

S. Bertolucci ◽

C. Berucci ◽

A.M. Bragadireanu ◽

...

Keyword(s):

Pauli Exclusion Principle ◽

Exclusion Principle

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Born–Infeld extension of Lovelock brane gravity in the system of M0-branes and its application for the emergence of Pauli exclusion principle in BIonic superconductors

Physics Letters A ◽

10.1016/j.physleta.2016.05.015 ◽

2016 ◽

Vol 380 (29-30) ◽

pp. 2247-2259 ◽

Cited By ~ 14

Author(s):

Alireza Sepehri

Keyword(s):

Pauli Exclusion Principle ◽

Exclusion Principle ◽

Brane Gravity

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Thermonuclear plasma conditions in stellar interiors

Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences ◽

10.1098/rsta.1981.0092 ◽

1981 ◽

Vol 300 (1456) ◽

pp. 641-648

Keyword(s):

Nuclear Reactions ◽

Pauli Exclusion Principle ◽

Significant Rise ◽

Exclusion Principle ◽

Reaction Products ◽

Thermonuclear Reactions ◽

Radiated Energy ◽

Large Numbers ◽

Stellar Interiors ◽

Late Stages

Thermonuclear reactions provide the main source of radiated energy for stars and they are also believed to be responsible for the production of most of the heavy elements in the Universe. The thermonuclear plasma is confined by the force of gravitation and for most of a star’s history the reactions occur slowly and steadily. In some circumstances, the properties of a star change very rapidly and explosive nuclear reactions occur. In very dense stellar interiors the energy states available to electrons may be limited by the Pauli exclusion principle. When thermonuclear reactions start in such a degenerate gas, a rise in temperature is not accompanied by a significant rise in pressure and as a result there may be a runaway increase in reaction rate. In contrast, when reactions start in a non-degenerate gas, there is normally an effective thermostat. A star is usually opaque to reaction products, so that there is no problem in maintaining the reaction temperature, but at late stages of stellar evolution nuclear or elementary particle reactions may produce large numbers of neutrinos and antineutrinos that do escape.

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