Relativistic Breit–Wigner distribution
The relativistic Breit–Wigner distribution (after the 1936 nuclear resonance formula of Gregory Breit and Eugene Wigner) is a continuous probability distribution with the following probability density function, where k is a constant of proportionality, equal to with (This equation is written using natural units, ħ = c = 1.) In the limit of vanishing width, Γ→0, the particle becomes stable as the Lorentzian distribution f sharpens infinitely to 2M δ(E2−M2). .(Further information: Cauchy distribution)
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Relativistic Breit–Wigner distribution
The relativistic Breit–Wigner distribution (after the 1936 nuclear resonance formula of Gregory Breit and Eugene Wigner) is a continuous probability distribution with the following probability density function, where k is a constant of proportionality, equal to with (This equation is written using natural units, ħ = c = 1.) In the limit of vanishing width, Γ→0, the particle becomes stable as the Lorentzian distribution f sharpens infinitely to 2M δ(E2−M2). .(Further information: Cauchy distribution)
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La distribución relativista de ...... es la distribución de Cauchy.
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La distribuzione Breit–Wigner ...... una forza esterna sinusoidale.
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The relativistic Breit–Wigner ...... rmation: Cauchy distribution)
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Wzór Breita-Wignera, rozkład B ...... ansowej opada o wiele wolniej.
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Формула Брейта — Вигнера или р ...... по времени входной мощности .
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719,796,609
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La distribución relativista de ...... es la distribución de Cauchy.
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La distribuzione Breit–Wigner ...... rgia tracci la forma della dis
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The relativistic Breit–Wigner ...... rmation: Cauchy distribution)
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Wzór Breita-Wignera, rozkład B ...... bieństwa rozkładem Cauchy’ego.
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Формула Брейта — Вигнера или р ...... онечно острым 2M δ(Е2 - М2). .
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Distribución de Breit-Wigner relativista
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Distribuzione Breit-Wigner relativistica
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Relativistic Breit–Wigner distribution
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Wzór Breita-Wignera
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Формула Брейта — Вигнера
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