Abstract:Motivated by improving the understanding of the quantum-to-classical transition we use a simple model of classical discrete interactions for studying the discrete-to-continuous transition in the classical harmonic oscilator. A parallel is traced with gravity for stressing the relevance of such discrete interaction models. Fundamental interactions, according to quantum field theory, are realized through the exchange of interaction quanta-packets of matter-energy with defined quantum numbers, viz. momentum-energ… Show more
“…Let us consider that the field-generating particle (gravitational or electric) is at the origin of the considered coordinate system and that the test particle is in the position r 0 with momentum p 0 and that r 0 < 1 with δr j << 1, this ensures that the two particles are very close to each other (such as inside a nucleus). We will also consider δt j << 1, this ensures that the iterative process approaches the continuous fields picture as expected, it is important to note that there are analytic approaches in which the fields are considered as discrete, [17][18][19] is not the case in question. Defining the time increment as being constant, i.e., δt j ≡ ω > 0, equations ( 11) and ( 10) then become…”
In this work we propose an alternative semiclassical iterative approach to obtain the Yukawa Potential, where the temporal evolution is replaced by the number of iterations. In addition, our analytical approach was able to provide an exact value very close to the adopted semi-empirically for the Yukawa magnitude scale constant.
“…Let us consider that the field-generating particle (gravitational or electric) is at the origin of the considered coordinate system and that the test particle is in the position r 0 with momentum p 0 and that r 0 < 1 with δr j << 1, this ensures that the two particles are very close to each other (such as inside a nucleus). We will also consider δt j << 1, this ensures that the iterative process approaches the continuous fields picture as expected, it is important to note that there are analytic approaches in which the fields are considered as discrete, [17][18][19] is not the case in question. Defining the time increment as being constant, i.e., δt j ≡ ω > 0, equations ( 11) and ( 10) then become…”
In this work we propose an alternative semiclassical iterative approach to obtain the Yukawa Potential, where the temporal evolution is replaced by the number of iterations. In addition, our analytical approach was able to provide an exact value very close to the adopted semi-empirically for the Yukawa magnitude scale constant.
“…O vetor posição x n = x nî , muda continuamente, descrevendo uma trajetória poligonal. Nesta abordagem a velocidade (momento linear se quisermos dar um tratamento semi-clássico [24]) muda discretamente. As variáveis contínuas tempo e posição entram na descrição do movimento como se fossem parâmetros discretos somente porque esses eventos de iteração são nossos pontos de referência para a contagem do tempo.…”
Section: Abordagem Iterativa Para O Oscilador Harmônico Simplesunclassified
Resumo Neste trabalho propusemos uma abordagem iterativa analítica em que a evolução temporal foi substituída pelo número de iterações. E para o caso de um sistema massa-mola obtivemos sua velocidade e sua posição em função do tempo como somas parciais de séries que convergiram para as funções trigonométricas que são as soluções do oscilador harmônico simples.
“…At low values of n, this is sensible -we expect that the increased oscillations as we climb the eigenfunction ladder do indeed correspond to greater quantumness. However, this does not hold at high values of n. The correspondence principle dictates that the limit as n → ∞ of the harmonic oscillator [5] should yield a transition from quantum to classical behavior. As such, a monotonic increase in quantumness with n is not correct.…”
The negativity of a given state's Wigner function has been proposed as a measure of quantumness of that state in a unipartite system. This otherwise physically intuitive and useful phase-space measure however does not yield the right correspondence principle limit, and also turns out to yield infinite values of the infinite square well. We show that both these issues can be sensibly resolved using coarse-graining of the Wigner function.
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