Do quantum fluctuations really tip the pencil? A classical trigger mechanism

Abstract We revisit the classic “tipping pencil” instability, a rigid rod balanced upright on its tip and allowed to rotate in a vertical plane, long used as an introductory illustration of the quantum–classical boundary. In the standard semiclassical argument, the upright configuration is destabilized by minimal uncertainties in the initial angle and angular momentum, $$ \delta \theta $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>δ</mml:mi> <mml:mi>θ</mml:mi> </mml:mrow> </mml:math> and $$\delta L$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>δ</mml:mi> <mml:mi>L</mml:mi> </mml:mrow> </mml:math> , constrained by $$\delta \theta \,\delta L\gtrsim \hbar /2$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>δ</mml:mi> <mml:mi>θ</mml:mi> <mml:mspace/> <mml:mi>δ</mml:mi> <mml:mi>L</mml:mi> <mml:mo>≳</mml:mo> <mml:mi>ħ</mml:mi> <mml:mo>/</mml:mo> <mml:mn>2</mml:mn> </mml:mrow> </mml:math> , with $$\delta L\simeq I\delta \omega $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>δ</mml:mi> <mml:mi>L</mml:mi> <mml:mo>≃</mml:mo> <mml:mi>I</mml:mi> <mml:mi>δ</mml:mi> <mml:mi>ω</mml:mi> </mml:mrow> </mml:math> . For a homogeneous cylinder of length $$a=10\,\textrm{cm}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>a</mml:mi> <mml:mo>=</mml:mo> <mml:mn>10</mml:mn> <mml:mspace/> <mml:mtext>cm</mml:mtext> </mml:mrow> </mml:math> and mass $$m=100\,\textrm{g}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>m</mml:mi> <mml:mo>=</mml:mo> <mml:mn>100</mml:mn> <mml:mspace/> <mml:mtext>g</mml:mtext> </mml:mrow> </mml:math> , the resulting uncertainty-based initial scales are extremely small and lead to tipping times of order a few seconds. We show, however, that quantum fluctuations are not required as the dominant physical seed for a finite tipping time. A purely classical microscopic perturbation, such as the angular-momentum transfer from a single elastic collision with a residual $$ O_{2}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>O</mml:mi> <mml:mn>2</mml:mn> </mml:msub> </mml:math> molecule under ultrahigh-vacuum conditions, already provides a conservative seed for the exponential instability. Using conservation of angular momentum, we estimate an imparted angular velocity $$ \omega _{0,O_{2}}\simeq 1.5\times 10^{-20}\,\textrm{s}^{-1}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:msub> <mml:mi>ω</mml:mi> <mml:mrow> <mml:mn>0</mml:mn> <mml:mo>,</mml:mo> <mml:msub> <mml:mi>O</mml:mi> <mml:mn>2</mml:mn> </mml:msub> </mml:mrow> </mml:msub> <mml:mo>≃</mml:mo> <mml:mn>1.5</mml:mn> <mml:mo>×</mml:mo> <mml:msup> <mml:mn>10</mml:mn> <mml:mrow> <mml:mo>-</mml:mo> <mml:mn>20</mml:mn> </mml:mrow> </mml:msup> <mml:mspace/> <mml:msup> <mml:mtext>s</mml:mtext> <mml:mrow> <mml:mo>-</mml:mo> <mml:mn>1</mml:mn> </mml:mrow> </mml:msup> </mml:mrow> </mml:math> , about five orders of magnitude smaller than the uncertainty-based angular-velocity scale, yet still sufficient to produce a macroscopic fall because the dependence on the seed is only logarithmic. We also include the more natural classical estimate due to thermal angular fluctuations. At room temperature, equipartition gives $$\theta _{\textrm{th}}\sim 3\times 10^{-10}\,\textrm{rad}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:msub> <mml:mi>θ</mml:mi> <mml:mtext>th</mml:mtext> </mml:msub> <mml:mo>∼</mml:mo> <mml:mn>3</mml:mn> <mml:mo>×</mml:mo> <mml:msup> <mml:mn>10</mml:mn> <mml:mrow> <mml:mo>-</mml:mo> <mml:mn>10</mml:mn> </mml:mrow> </mml:msup> <mml:mspace/> <mml:mtext>rad</mml:mtext> </mml:mrow> </mml:math> and $$\omega _{\textrm{th}}\sim 3.5\times 10^{-9}\,\textrm{s}^{-1}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:msub> <mml:mi>ω</mml:mi> <mml:mtext>th</mml:mtext> </mml:msub> <mml:mo>∼</mml:mo> <mml:mn>3.5</mml:mn> <mml:mo>×</mml:mo> <mml:msup> <mml:mn>10</mml:mn> <mml:mrow> <mml:mo>-</mml:m

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Journal
The European Physical Journal Plus
Published
2026-06-28
DOI
https://doi.org/10.1140/epjp/s13360-026-07964-3
Primary Topic
Quantum chaos and dynamical systems
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article
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article

Do quantum fluctuations really tip the pencil? A classical trigger mechanism

J. Ricardo de Sousa
The European Physical Journal Plus
Quantum chaos and dynamical systems
article

Do quantum fluctuations really tip the pencil? A classical trigger mechanism

J. Ricardo de Sousa
article en

Abstract

Abstract We revisit the classic “tipping pencil” instability, a rigid rod balanced upright on its tip and allowed to rotate in a vertical plane, long used as an introductory illustration of the quantum–classical boundary. In the standard semiclassical argument, the upright configuration is destabilized by minimal uncertainties in the initial angle and angular momentum, $$ \delta \theta $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>δ</mml:mi> <mml:mi>θ</mml:mi> </mml:mrow> </mml:math> and $$\delta L$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>δ</mml:mi> <mml:mi>L</mml:mi> </mml:mrow> </mml:math> , constrained by $$\delta \theta \,\delta L\gtrsim \hbar /2$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>δ</mml:mi> <mml:mi>θ</mml:mi> <mml:mspace/> <mml:mi>δ</mml:mi> <mml:mi>L</mml:mi> <mml:mo>≳</mml:mo> <mml:mi>ħ</mml:mi> <mml:mo>/</mml:mo> <mml:mn>2</mml:mn> </mml:mrow> </mml:math> , with $$\delta L\simeq I\delta \omega $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>δ</mml:mi> <mml:mi>L</mml:mi> <mml:mo>≃</mml:mo> <mml:mi>I</mml:mi> <mml:mi>δ</mml:mi> <mml:mi>ω</mml:mi> </mml:mrow> </mml:math> . For a homogeneous cylinder of length $$a=10\,\textrm{cm}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>a</mml:mi> <mml:mo>=</mml:mo> <mml:mn>10</mml:mn> <mml:mspace/> <mml:mtext>cm</mml:mtext> </mml:mrow> </mml:math> and mass $$m=100\,\textrm{g}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>m</mml:mi> <mml:mo>=</mml:mo> <mml:mn>100</mml:mn> <mml:mspace/> <mml:mtext>g</mml:mtext> </mml:mrow> </mml:math> , the resulting uncertainty-based initial scales are extremely small and lead to tipping times of order a few seconds. We show, however, that quantum fluctuations are not required as the dominant physical seed for a finite tipping time. A purely classical microscopic perturbation, such as the angular-momentum transfer from a single elastic collision with a residual $$ O_{2}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>O</mml:mi> <mml:mn>2</mml:mn> </mml:msub> </mml:math> molecule under ultrahigh-vacuum conditions, already provides a conservative seed for the exponential instability. Using conservation of angular momentum, we estimate an imparted angular velocity $$ \omega _{0,O_{2}}\simeq 1.5\times 10^{-20}\,\textrm{s}^{-1}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:msub> <mml:mi>ω</mml:mi> <mml:mrow> <mml:mn>0</mml:mn> <mml:mo>,</mml:mo> <mml:msub> <mml:mi>O</mml:mi> <mml:mn>2</mml:mn> </mml:msub> </mml:mrow> </mml:msub> <mml:mo>≃</mml:mo> <mml:mn>1.5</mml:mn> <mml:mo>×</mml:mo> <mml:msup> <mml:mn>10</mml:mn> <mml:mrow> <mml:mo>-</mml:mo> <mml:mn>20</mml:mn> </mml:mrow> </mml:msup> <mml:mspace/> <mml:msup> <mml:mtext>s</mml:mtext> <mml:mrow> <mml:mo>-</mml:mo> <mml:mn>1</mml:mn> </mml:mrow> </mml:msup> </mml:mrow> </mml:math> , about five orders of magnitude smaller than the uncertainty-based angular-velocity scale, yet still sufficient to produce a macroscopic fall because the dependence on the seed is only logarithmic. We also include the more natural classical estimate due to thermal angular fluctuations. At room temperature, equipartition gives $$\theta _{\textrm{th}}\sim 3\times 10^{-10}\,\textrm{rad}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:msub> <mml:mi>θ</mml:mi> <mml:mtext>th</mml:mtext> </mml:msub> <mml:mo>∼</mml:mo> <mml:mn>3</mml:mn> <mml:mo>×</mml:mo> <mml:msup> <mml:mn>10</mml:mn> <mml:mrow> <mml:mo>-</mml:mo> <mml:mn>10</mml:mn> </mml:mrow> </mml:msup> <mml:mspace/> <mml:mtext>rad</mml:mtext> </mml:mrow> </mml:math> and $$\omega _{\textrm{th}}\sim 3.5\times 10^{-9}\,\textrm{s}^{-1}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:msub> <mml:mi>ω</mml:mi> <mml:mtext>th</mml:mtext> </mml:msub> <mml:mo>∼</mml:mo> <mml:mn>3.5</mml:mn> <mml:mo>×</mml:mo> <mml:msup> <mml:mn>10</mml:mn> <mml:mrow> <mml:mo>-</mml:m

The European Physical Journal PlusVol. 141(6)
Universidade Federal do Amazonas (BR)
Universidade Federal do Amazonas, Coordenação de Aperfeiçoamento de Pessoal de Nível Superior
Openalex Percentile: Top 7%
Quantum chaos and dynamical systems
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