P1-VL:连接物理奥林匹克竞赛中的视觉感知与科学推理

High School Physics Olympiad Benchmark (HiPhO)

P1-VL生态系统

首个物理奥赛基准测试:HiPhO

课程强化学习

PhysicsMinions系统架构
图三:PhysicsMinions 协同进化多智能体系统概览,展示了三个模块之间的交互流程。

协同进化的多智能体系统:PhysicsMinions

评测结果

P1-VL 模型展现顶级物理推理能力

HiPhO Leaderboard
图四:P1系列模型在 HiPhO 基准测试上的综合表现,包括与开源和闭源模型的对比。

卓越的科学推理能力

FrontierScience-Olympiad Benchmark

通专融合,P1-VL模型通用能力持续提升

P1-VL-30B-A3B vs Qwen3-VL-30B-A3B Performance Comparison
P1-VL-235B-A22B vs Qwen3-VL-235B-A22B-Thinking Performance Comparison

案例研究

Background

This problem aims to study the peculiar physics of galaxies, such as their dynamics and structure. In particular, we explain how to measure the mass distribution of our galaxy from the inside. For this we will focus on hydrogen, its main constituent.

figure7

Part D - Tully-Fisher relation and MOND theory

The flat external velocity curve of NGC 6946 in Fig. 1 is a common property of spiral galaxies, as can be seen in Fig. 4 (left). Plotting the external constant velocity value $v_{c,\infty}$ as a function of the measured total mass $𝑀_{tot}$ of each galaxy gives an interesting correlation called the Tully-Fischer relation, see Fig. 4 (right)

figure7

Question

Let 𝑚 be a mass on a circular orbit of radius $𝑟$ with velocity $𝑣_{𝑐,\infty}$ in the gravity field of a fixed mass $𝑀$. Within the MOND theory, with 𝑎 ≪ $𝑎_0$ , determine the Tully-Fischer exponent. Using data for NGC 6946 and/or Tully-Fischer law, calculate $𝑎_0$ to show that MOND operates in the correct regime.
P1-VL
0.8 pt
答案
(1) $\gamma_{\text{MOND}} = 4$
(2) $a_0 = \frac{v_{c,\infty}^4}{G M_{\text{tot}}}$
(3) $a_0 = 1.2 \times 10^{-10}$ m/s²
评估标准
Award 0.1 pt if the answer considers the hypothesis $a \ll a_0$. Otherwise, award 0 pt.
Award 0.1 pt if the answer applies the Newton's second law and derives $G \frac{M}{r^2} m = m \frac{a^2}{a_0}$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly gives the expression for $v_{c,\infty}$ as $v_{c,\infty} = (a_0 G M)^{1/4}$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly gives the numerical value for $\gamma_{\text{MOND}}$ as $\gamma_{\text{MOND}} = 4$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly gives the numerical value for $\log_{10}(v_{c,\infty} / {1 \mathrm{km/s}}) = 2.2$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly gives the numerical value for $\log_{10}(M_{\text{tot}} / M_{\odot}) = 10.5$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly gives the expression for $a_0$ as $a_0 = \frac{v_{c,\infty}^4}{G M_{\text{tot}}}$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly gives the numerical value for $a_0$ within the range $[10^{-10.5}, 10^{-9.5}]$. Otherwise, award 0 pt.
总分: 0.8 pt

To address the problem, we examine the MOND theory's implications for the Tully-Fischer relation and derive the necessary expressions and numerical values based on the given data.

(1) Tully-Fischer Exponent under MOND

In MOND theory, the gravitational force is related to the acceleration through the modified second law:

$$F = m \mu\left(\frac{a}{a_0}\right) a,$$

where $\mu(x) = \frac{x}{1+x}$ and $a_0$ is the critical acceleration. In the deep-MOND regime ($a \ll a_0$), $\mu(a/a_0) \approx a/a_0$, leading to:

$$F = \frac{m a^2}{a_0}.$$

For a circular orbit, the centripetal acceleration is $a = v^2 / r$, and the gravitational force is $F = G M m / r^2$. Equating these:

$$\frac{G M m}{r^2} = \frac{m (v^2 / r)^2}{a_0} \Rightarrow G M = \frac{v^4}{a_0}.$$

Solving for $M$, we obtain:

$$M = \frac{v^4}{G a_0}.$$

This implies that the total mass $M$ scales with the fourth power of the rotation velocity $v$. Therefore, the Tully-Fischer exponent is:

$$\boxed{4}$$

To verify that MOND operates in the correct regime for NGC 6946, we estimate $a_0$ using the observed flat rotation velocity $v_{c,\infty} = 150 \, \text{km/s} = 1.5 \times 10^5 \, \text{m/s}$ and the total baryonic mass inferred from the Tully-Fischer relation.

From Fig. 4, at $v_{c,\infty} = 150 \, \text{km/s}$, the corresponding total mass is approximately $M_{\text{tot}} = 3.16 \times 10^{10} \, M_\odot$. Converting to kilograms:

$$M = 3.16 \times 10^{10} \times 1.99 \times 10^{30} \approx 6.3 \times 10^{40} \, \text{kg}.$$

Using $G = 6.67 \times 10^{-11} \, \text{m}^3 \text{kg}^{-1} \text{s}^{-2}$, we calculate $a_0$:

$$a_0 = \frac{v_{c,\infty}^4}{G M} = \frac{(1.5 \times 10^5)^4}{6.67 \times 10^{-11} \times 6.3 \times 10^{40}}.$$

$$v^4 = (1.5)^4 \times 10^{20} = 5.06 \times 10^{20} \, \text{m}^4/\text{s}^4,$$

$$G M = 4.2 \times 10^{30} \, \text{m}^3/\text{s}^2,$$

$$a_0 = \frac{5.06 \times 10^{20}}{4.2 \times 10^{30}} \approx 1.2 \times 10^{-10} \, \text{m/s}^2.$$

This value matches the expected order of magnitude for $a_0$, confirming that the observed acceleration $a = v^2 / r$ in the outer regions of NGC 6946 (e.g., $a \sim 7 \times 10^{-11} \, \text{m/s}^2$ at $r = 10 \, \text{kpc}$) is in the MOND regime ($a \ll a_0$).

(2) Expression for $a_0$

From the MOND analysis for circular motion in the deep-MOND regime, we derived the relation:

$$M = \frac{v_{c,\infty}^4}{G a_0}.$$

Solving for $a_0$, the expression for the critical acceleration is:

$$\boxed{a_0 = \frac{v_{c,\infty}^4}{G M_{\text{tot}}}}$$

This expression links the critical MOND acceleration to the observed rotation velocity and the total baryonic mass of the galaxy.

(3) Numerical Value of $a_0$

Using the observed values for NGC 6946:

  • $v_{c,\infty} = 1.5 \times 10^5 \, \text{m/s}$,
  • $M_{\text{tot}} \approx 6.3 \times 10^{40} \, \text{kg}$,
  • $G = 6.67 \times 10^{-11} \, \text{m}^3 \text{kg}^{-1} \text{s}^{-2}$,

we compute:

$$a_0 = \frac{(1.5 \times 10^5)^4}{6.67 \times 10^{-11} \times 6.3 \times 10^{40}} = \frac{5.06 \times 10^{20}}{4.2 \times 10^{30}} \approx 1.2 \times 10^{-10} \, \text{m/s}^2.$$

Thus, the numerical value of $a_0$ is:

$$\boxed{1.2 \times 10^{-10}}$$

This value is consistent with the MOND prediction and confirms that the galaxy operates in the MOND regime.

Final Answers

(1) The Tully-Fischer exponent within MOND is $\boxed{4}$. Using NGC 6946 data, the calculation confirms that MOND operates in the correct regime.

(2) The expression for $a_0$ is $\boxed{a_0 = \frac{v_{c,\infty}^4}{G M_{\text{tot}}}}$.

(3) The numerical value of $a_0$ is $\boxed{1.2 \times 10^{-10}}$ m/s².

Gemini-3-Pro
0.5 pt
答案
(1) $\gamma_{\text{MOND}} = 4$
(2) $a_0 = \frac{v_{c,\infty}^4}{GM}$
(3) $a_0 = 3.8 \times 10^{-9}$ m/s²
评估标准
Award 0.1 pt if the answer considers the hypothesis $a \ll a_0$. Otherwise, award 0 pt.
Award 0.1 pt if the answer applies the Newton's second law and derives $G \frac{M}{r^2} m = m \frac{a^2}{a_0}$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly gives the expression for $v_{c,\infty}$ as $v_{c,\infty} = (a_0 G M)^{1/4}$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly gives the numerical value for $\gamma_{\text{MOND}}$ as $\gamma_{\text{MOND}} = 4$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly gives the numerical value for $\log_{10}(v_{c,\infty} / {1 \mathrm{km/s}}) = 2.2$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly gives the numerical value for $\log_{10}(M_{\text{tot}} / M_{\odot}) = 10.5$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly gives the expression for $a_0$ as $a_0 = \frac{v_{c,\infty}^4}{G M_{\text{tot}}}$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly gives the numerical value for $a_0$ within the range $[10^{-10.5}, 10^{-9.5}]$. Otherwise, award 0 pt.
总分: 0.5 pt
(1) Determination of Tully-Fisher exponent $\gamma_{\text{MOND}}$:

Consider a mass $m$ in a circular orbit of radius $r$ around a galaxy of baryonic mass $M$. Newton's gravitational force is $F_N = \frac{GMm}{r^2}$. According to MOND theory, in the low acceleration regime ($a \ll a_0$), the force is modified such that $F_N = m \mu(\frac{a}{a_0}) a$. Approximating $\mu(x) \approx x$ for $x \ll 1$:

$$\frac{GMm}{r^2} = m \left( \frac{a}{a_0} \right) a = \frac{m a^2}{a_0}$$

For circular motion, the centripetal acceleration is $a = \frac{v^2}{r}$. Substituting this into the force equation:

$$\frac{GM}{r^2} = \frac{1}{a_0} \left( \frac{v^2}{r} \right)^2 = \frac{v^4}{a_0 r^2}$$

Simplifying by canceling $r^2$:

$$GM = \frac{v^4}{a_0} \implies M = \frac{1}{G a_0} v^4$$

This matches the Tully-Fisher relation $M \propto v^\gamma$ with an exponent:

$$\gamma_{\text{MOND}} = 4$$

Check of MOND regime: Using the data for NGC 6946 from Fig. 1(B): The flat rotation velocity is approximately $v_{c,\infty} \approx 165 \, \mathrm{km/s}$. At the outer edge of the data, $r \approx 11 \, \mathrm{kpc}$. The observed acceleration is:

$$a_{\text{obs}} = \frac{v_{c,\infty}^2}{r} = \frac{(1.65 \times 10^5 \, \mathrm{m/s})^2}{11 \times 3.09 \times 10^{19} \, \mathrm{m}} \approx \frac{2.72 \times 10^{10}}{3.40 \times 10^{20}} \approx 0.8 \times 10^{-10} \, \mathrm{m/s^2}$$

This value is of the order of $a_0 = 10^{-10} \, \mathrm{m/s^2}$. Specifically, if $a_0 \approx 1.2 \times 10^{-10} \mathrm{m/s^2}$ (standard value) or slightly higher (as calculated below), the condition $a_{\text{obs}} \lesssim a_0$ holds, confirming the galaxy's outer region is in the MOND regime.

$$\boxed{4}$$

(2) Expression for $a_0$:

From the derived MOND relation $GM = \frac{v_{c,\infty}^4}{a_0}$, we can write $a_0$ as:

$$a_0 = \frac{v_{c,\infty}^4}{GM}$$

Here, $M$ represents the total baryonic mass. Based on the problem description, the red curve in Fig. 1(B) represents the predicted Keplerian velocity due to the visible mass $M$. Let $v_{\text{pred}}(r)$ be the velocity from the red curve at a large radius $r$. Then $v_{\text{pred}}^2 = \frac{GM}{r}$, so $GM = r v_{\text{pred}}^2$. Substituting this into the expression for $a_0$:

$$a_0 = \frac{v_{c,\infty}^4}{r v_{\text{pred}}(r)^2}$$

$$\boxed{a_0 = \frac{v_{c,\infty}^4}{GM}}$$

(3) Numerical value of $a_0$:

We use the data from Fig. 1(B) at a large radius, for example, $r = 10 \, \mathrm{kpc}$.

  • Observed velocity (flat part): $v_{c,\infty} \approx 165 \, \mathrm{km/s} = 1.65 \times 10^5 \, \mathrm{m/s}$.
  • Predicted Newtonian velocity (red curve): $v_{\text{pred}} \approx 25 \, \mathrm{km/s} = 2.5 \times 10^4 \, \mathrm{m/s}$.
  • Radius: $r = 10 \, \mathrm{kpc} = 10 \times 3.09 \times 10^{19} \, \mathrm{m} = 3.09 \times 10^{20} \, \mathrm{m}$.

Using the derived formula with $GM = r v_{\text{pred}}^2$:

$$a_0 = \frac{(1.65 \times 10^5)^4}{(3.09 \times 10^{20}) (2.5 \times 10^4)^2}$$

$$a_0 = \frac{7.41 \times 10^{20}}{3.09 \times 10^{20} \times 6.25 \times 10^8}$$

$$a_0 = \frac{7.41 \times 10^{20}}{1.93 \times 10^{29}} \approx 3.8 \times 10^{-9} \, \mathrm{m/s^2}$$

(Note: This value is higher than the standard $a_0 \approx 1.2 \times 10^{-10} \mathrm{m/s^2}$, likely because the red curve model considers only the bulge mass, underestimating the total baryonic mass $M$. However, based on the provided curves, this is the calculated value.)

$$\boxed{3.8 \times 10^{-9}}$$

GPT-5.2
0.5 pt
答案
(1) $\gamma_{\text{MOND}} = 4$
(2) $a_0 = \frac{v_{c,\infty}^2}{R}$
(3) $a_0 = 1.0 \times 10^{-10}$ m/s²
评估标准
Award 0.1 pt if the answer considers the hypothesis $a \ll a_0$. Otherwise, award 0 pt.
Award 0.1 pt if the answer applies the Newton's second law and derives $G \frac{M}{r^2} m = m \frac{a^2}{a_0}$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly gives the expression for $v_{c,\infty}$ as $v_{c,\infty} = (a_0 G M)^{1/4}$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly gives the numerical value for $\gamma_{\text{MOND}}$ as $\gamma_{\text{MOND}} = 4$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly gives the numerical value for $\log_{10}(v_{c,\infty} / {1 \mathrm{km/s}}) = 2.2$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly gives the numerical value for $\log_{10}(M_{\text{tot}} / M_{\odot}) = 10.5$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly gives the expression for $a_0$ as $a_0 = \frac{v_{c,\infty}^4}{G M_{\text{tot}}}$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly gives the numerical value for $a_0$ within the range $[10^{-10.5}, 10^{-9.5}]$. Otherwise, award 0 pt.
总分: 0.5 pt

In the MOND theory, for very low accelerations ($a \ll a_0$), the interpolation function is approximated by $\mu(x) \approx x$, where $x = a/a_0$. Newton's second law $\vec{F} = m \mu(a/a_0) \vec{a}$ becomes:

$$F = m \frac{a}{a_0} a = \frac{m a^2}{a_0}$$

For a mass $m$ on a circular orbit of radius $r$ with velocity $v$, the acceleration is $a = v^2/r$. The gravitational force is $F = \frac{G M m}{r^2}$. Substituting these into the modified law:

$$\frac{G M m}{r^2} = \frac{m}{a_0} \left( \frac{v^2}{r} \right)^2 = \frac{m v^4}{a_0 r^2}$$

Simplifying by canceling $m$ and $r^2$:

$$G M = \frac{v^4}{a_0} \implies M = \frac{1}{G a_0} v^4$$

The Tully-Fisher relation is of the form $M \propto v^\gamma$. Comparing the two, we find the exponent:

$$\gamma_{\text{MOND}} = 4$$

To check the regime, we calculate the characteristic acceleration of the galaxy NGC 6946 using the provided data. From Fig. 1(B), the rotation curve flattens at a velocity $v_{c,\infty} \approx 170 \, \text{km/s}$. From Fig. 1(A), the visible disk of the galaxy has a width of $18 \, \text{kpc}$, corresponding to a radius $R \approx 9 \, \text{kpc}$. The acceleration $a$ at the edge of the visible galaxy is:

$$a = \frac{v_{c,\infty}^2}{R}$$

Using the values $v_{c,\infty} = 1.70 \times 10^5 \, \text{m/s}$ and $R = 9 \times 3.09 \times 10^{19} \, \text{m} \approx 2.78 \times 10^{20} \, \text{m}$:

$$a \approx \frac{(1.70 \times 10^5)^2}{2.78 \times 10^{20}} = \frac{2.89 \times 10^{10}}{2.78 \times 10^{20}} \approx 1.04 \times 10^{-10} \, \text{m/s}^2$$

This calculated acceleration is of the order of $10^{-10} \, \text{m/s}^2$, matching the given scale for $a_0$. Since the acceleration in the outer regions ($a \sim 10^{-10}$) is comparable to or less than $a_0$, MOND effects are significant, and the approximation used ($a \lesssim a_0$) is valid for the flat part of the curve.

$$\boxed{\gamma_{\text{MOND}} = 4}$$

Based on the estimation using the galaxy's kinematic data at the optical radius:

$$\boxed{a_0 = \frac{v_{c,\infty}^2}{R}}$$

Using the values $v_{c,\infty} = 170 \, \text{km/s}$ and $R = 9 \, \text{kpc}$:

$$a_0 = \frac{(170 \times 10^3)^2}{9 \times 3.09 \times 10^{19}} \approx 1.04 \times 10^{-10} \, \text{m/s}^2$$

Rounding to two significant figures consistent with the reading of the graph:

$$\boxed{1.0 \times 10^{-10}}$$

背景

In 1765, British clockmaker James Cox invented a clock whose only source of energy is the fluctuations in atmospheric pressure. Cox's clock used two vessels containing mercury. Changes in atmospheric pressure caused mercury to move between the vessels, and the two vessels to move relative to each other. This movement acted as an energy source for the actual clock.

figure1
Fig. 1. Artistic view of Cox's clock

We propose an analysis of this device. Throughout, we assume that

  • the Earth's gravitational field $\vec{g} = -g\vec{u_{z}}$ is uniform with $g = 9.8 \mathrm{m} \cdot \mathrm{s}^{-2}$ and $\vec{u_{z}}$ a unit vector;
  • all liquids are incompressible and their density is denoted $\rho$;
  • no surface tension effects will be considered;
  • the variations of atmospheric pressure with altitude are neglected;
  • the surrounding temperature $T_{\mathrm{a}}$ is uniform and all transformations are isothermal.

A. Pulling on a submerged tube

We first consider a bath of water that occupies the semi-infinite space $z \leq 0$. The air above it is at a pressure $P_{\text{a}} = P_0$. A cylindrical vertical tube of length $H = 1 \text{m}$, cross-sectional area $S = 10 \text{cm}^2$ and mass $m = 0.5 \text{kg}$ is dipped into the bath. The bottom of the tube is open, and the top end of the tube is closed. We denote $h$ the altitude of the top of the tube and $z_l$ that of the water inside the tube. The thickness of the tube walls is neglected.

We start from the situation where the tube in Fig. 2 contains no gas and its top is at the bath level: in other words, $h = 0$ and $z_l = 0$ (case a). The tube is then slowly lifted until its bottom end reaches the bath level. The pulling force exerted on the tube is denoted $\vec{F} = F\vec{u}_z$.

alt text
Fig. 2. Sketch of the tube in different configurations

A.2 Background

Three experiments are performed. In each, the tube is lifted from the initial state shown in Fig. 2(a) under the conditions specified in Table 1.

alt text
Table 1. Experimental conditions and numerical values of physical quantities for each experiment
($P_{\text{sat}}$ designates the saturated vapour pressure of the pure fluid)

In each case, we study the evolution of the force $F$ that must be applied in order to maintain the tube in equilibrium at an altitude $h$, the external pressure being fixed at $P_{\text{a}} = P_0 = 1.000 \times 10^5 \text{Pa}$. Two different behaviours are possible

alt text

Question A.1

For the configuration shown in Fig. 2 (case b), express the pressure $P_w$ in the water at the top of the tube. Also express the force $\vec{F}$ necessary to maintain the tube at this position. Expressions must be written in terms of $P_0, \rho, m, S, h, g$ and $\vec{u}_z$.

Question A.2

For each experiment, complete the table in the answer sheet to indicate the expected behaviour and the numerical values for $F_{\text{max}}$ and for $h^{\star}$ (when pertinent), where $F_{\text{max}}$ and $h^{\star}$ are defined in the figures illustrating the two behaviours.

A.1 模型答案

P1-VL
0.2 pt
答案
(1) $P_{\mathrm{w}} = P_0 - \rho g h$
(2) $\vec{F} = \left( m g + \rho g h S \right) \vec{u_{z}}$
评估标准
Award 0.1 pt if the answer correctly gives the expression of $P_w$ as a function of $P_a$ or $P_0$: $P_w = P_a - \rho g h = P_0 - \rho g h$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly derives the expression of $\vec{F}$ as $\vec{F} = [m + \rho S h] g \vec{u_{z}}$. Otherwise, award 0 pt.
总分: 0.2 pt

To analyze the situation for case b in Cox's timepiece, we consider the vertical tube of length $H$, cross-sectional area $S$, and mass $m$, lifted so that its bottom end is at the bath surface ($z = 0$) and its top is at altitude $h$. In this configuration, the water level inside the tube is at the same height as the top of the tube, i.e., $z_\ell = h$, indicating that the tube is completely filled with water.

(1) Pressure at the Top of the Tube

The tube is sealed at the top and open at the bottom, and the water inside is in hydrostatic equilibrium. The pressure at the bottom of the tube (at $z = 0$) must equal the atmospheric pressure $P_0$, as the tube is open to the bath at this level.

Using the hydrostatic pressure law, the pressure at any height $z$ inside the water column is given by:

$$P(z) = P_0 - \rho g z$$

At the top of the tube, where $z = h$, the pressure in the water is:

$$P_{\rm w} = P_0 - \rho g h$$

This result reflects that the pressure at the top of the water column is reduced by the weight of the water column of height $h$.

(2) Force Required to Maintain the Tube in Equilibrium

To determine the force $\vec{F}$ necessary to hold the tube in place, we perform a force balance on the tube alone.

Forces on the Tube:

  • Gravitational force: The tube has a mass $m$, so its weight is $-mg\vec{u_z}$.
  • Pressure forces:
    • The atmospheric pressure $P_0$ acts downward on the top cap of the tube, exerting a force $-P_0 S \vec{u_z}$.
    • The water pressure $P_{\rm w}$ at the top of the tube acts upward on the inner surface of the cap, exerting a force $+P_{\rm w} S \vec{u_z}$.

Thus, the net pressure force on the tube is:

$$(P_{\rm w} - P_0) S \vec{u_z} = -\rho g h S \vec{u_z}$$

This is a downward force due to the pressure difference between the outside atmosphere and the water column inside the tube.

  • Applied force: $\vec{F}$ is applied upward to maintain equilibrium.

Equilibrium Condition:

The net force on the tube must be zero:

$$\vec{F} + (P_{\rm w} - P_0) S \vec{u_z} - m g \vec{u_z} = \vec{0}$$

Substituting $P_{\rm w} = P_0 - \rho g h$:

$$\vec{F} - \rho g h S \vec{u_z} - m g \vec{u_z} = \vec{0}$$

$$\Rightarrow \vec{F} = (m g + \rho g h S) \vec{u_z}$$

This result is physically intuitive: the force required to hold the tube in place must counteract both the tube's own weight and the net downward pressure force due to the difference between atmospheric pressure and the reduced pressure at the top of the water column.

Final Answers

(1) The pressure in the water at the top of the tube is:

$$\boxed{P_{\mathrm{w}} = P_0 - \rho g h}$$

(2) The force required to maintain the tube in equilibrium is:

$$\boxed{\vec{F} = \left( m g + \rho g h S \right) \vec{u_{z}}}$$

Gemini-3-Pro
0.2 pt
答案
(1) $P_{\mathrm{w}} = P_{0} - \rho g h$
(2) $\vec{F} = (m + \rho S h)g \vec{u_{z}}$
评估标准
Award 0.1 pt if the answer correctly gives the expression of $P_w$ as a function of $P_a$ or $P_0$: $P_w = P_a - \rho g h = P_0 - \rho g h$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly derives the expression of $\vec{F}$ as $\vec{F} = [m + \rho S h] g \vec{u_{z}}$. Otherwise, award 0 pt.
总分: 0.2 pt

(1) Since the tube is slowly lifted and contains no gas, the water fills the tube up to the top inner surface as long as the pressure remains above the vapor pressure (which is the case here given the dimensions and atmospheric pressure). Thus, the water level inside the tube is $z_{\ell} = h$.

The pressure in the stationary water column varies with height according to the hydrostatic law. Taking the pressure at the surface of the bath ($z=0$) as the atmospheric pressure $P_{0}$, the pressure $P_{\mathrm{w}}$ at the altitude $h$ inside the water column is given by:

$$P_{\mathrm{w}} = P_{0} - \rho g h$$

$\boxed{P_{\mathrm{w}} = P_{0} - \rho g h}$

(2) To find the force $\vec{F}$ necessary to maintain the tube in equilibrium, we consider the balance of forces acting on the tube. The tube has mass $m$, so the gravitational force is $-mg\vec{u_{z}}$. The external lifting force is $\vec{F}$.

The pressure forces acting on the tube are due to the atmosphere on the outer top surface and the water on the inner top surface. The thickness of the walls is neglected, so the area for both surfaces is $S$. The side walls are vertical, so pressure forces on them cancel horizontally and have no vertical component.

  • Force from atmospheric pressure on the top (downward): $\vec{F}_{\text{air}} = -P_{0} S \vec{u_{z}}$.
  • Force from water pressure on the top inside (upward): $\vec{F}_{\text{water}} = P_{\mathrm{w}} S \vec{u_{z}} = (P_{0} - \rho g h) S \vec{u_{z}}$.

The equilibrium condition $\sum \vec{F} = \vec{0}$ gives:

$$\vec{F} - mg\vec{u_{z}} - P_{0} S \vec{u_{z}} + (P_{0} - \rho g h) S \vec{u_{z}} = \vec{0}$$

$$\vec{F} = \left( mg + P_{0} S - P_{0} S + \rho g h S \right) \vec{u_{z}}$$

$$\vec{F} = (mg + \rho S h g) \vec{u_{z}}$$

Alternatively, one can consider that the external force must support the weight of the tube plus the weight of the suspended water column of height $h$ (volume $Sh$) pulled up above the bath level.

Weight of tube: $mg$.

Weight of lifted water: $\rho (Sh) g$.

Total magnitude: $F = mg + \rho S h g$.

Direction is upward ($\vec{u_{z}}$).

$\boxed{\vec{F} = (m + \rho S h)g \vec{u_{z}}}$

Gemini-2.5-Pro
0.2 pt
答案
(1) $P_0 - \rho g h$
(2) $(mg + \rho g h S)\vec{u_z}$
评估标准
Award 0.1 pt if the answer correctly gives the expression of $P_w$ as a function of $P_a$ or $P_0$: $P_w = P_a - \rho g h = P_0 - \rho g h$. Otherwise, award 0 pt.
Award 0.1 pt if the answer correctly derives the expression of $\vec{F}$ as $\vec{F} = [m + \rho S h] g \vec{u_{z}}$. Otherwise, award 0 pt.
总分: 0.2 pt

Problem Solution: Tube Lifted from Water Bath

Part (1): Finding the pressure $P_w$ at the top of the tube

Step 1: Analyze the physical situation

The problem describes a cylindrical tube (length $H=1 \text{m}$, closed top, open bottom) initially filled with water and submerged such that its top is at the water surface ($h=0$). No gas is inside the tube. We study the configuration (Fig. 2b) where the tube's top is at height $h$ above the external water level.

Step 2: Determine the water level inside the tube, $z_l$

The space above the water column in the tube is a vacuum (no initial gas, neglect water vapor pressure). Atmospheric pressure $P_0$ supports a water column of maximum (barometric) height:

$$H_{\text{baro}} = \frac{P_0}{\rho g}$$

Using $P_0 \approx 1.013 \times 10^5 \text{Pa}$, $\rho \approx 1000 \text{kg/m}^3$, we get $H_{\text{baro}} \approx 10.3 \text{m}$. Since the tube length $H=1 \text{m} < 10.3 \text{m}$, atmospheric pressure keeps the tube fully filled with water. Thus:

$$z_l = h$$

Step 3: Calculate $P_w$ using hydrostatics

The hydrostatic principle for a static fluid: $P_2 = P_1 - \rho g (z_2 - z_1)$.

  • Point 1: External water surface ($z_1=0$, $P_1=P_0$)
  • Point 2: Top of the water column inside the tube ($z_2=h$, $P_2=P_w$)

Substituting gives:

$$P_w = P_0 - \rho g h$$

Part (2): Finding the force $\vec{F}$

Step 1: Define the system and identify external forces

Treat the tube + water inside as the system (static equilibrium, net force = 0). External forces:

  1. Pulling force: $\vec{F} = F \vec{u_z}$ (upward)
  2. Tube's weight: $\vec{W}_{\text{tube}} = -mg \vec{u_z}$ (downward)
  3. Water's weight (volume $V_w = S \cdot H$): $\vec{W}_{\text{water}} = -\rho S H g \vec{u_z}$ (downward)
  4. Atmospheric force on tube top: $\vec{F}_{\text{air}} = -P_0 S \vec{u_z}$ (downward)
  5. Water pressure force on tube bottom (height $z_{\text{bottom}} = h - H$, pressure $P(z_{\text{bottom}}) = P_0 - \rho g (h-H)$): $\vec{F}_{\text{water}} = (P_0 - \rho g (h-H)) S \vec{u_z}$ (upward)

Step 2: Apply static equilibrium (vertical direction)

$$\sum F_z = F - mg - \rho S H g - P_0 S + (P_0 - \rho g (h-H)) S = 0$$

Step 3: Solve for the magnitude of the force $F$

Let's simplify the equation:

$$F - mg - \rho g h S = 0 \implies F = mg + \rho g h S$$

Step 4: Express as a vector

The force acts upward (along $\vec{u_z}$):

$$\vec{F} = (mg + \rho g h S) \vec{u_z}$$

Final Check

  • $P_w$ decreases linearly with $h$; at $h=0$, $P_w = P_0$ (reasonable).
  • $F$ increases linearly with $h$; at $h=0$, $F=mg$ (supports only the tube's weight). The term $\rho g h S$ is the weight of the lifted water column.

Answers

(1) Pressure at the top of the tube:

$$\boxed{P_0 - \rho g h}$$

(2) Force to maintain equilibrium:

$$\boxed{(mg + \rho g h S)\vec{u_z}}$$

A.2 模型答案

P1-VL
0.8 pt
答案
Experiment 1: A, None, 14.7 N
Experiment 2: A, None, 14.4 N
Experiment 3: B, 2.1 cm, 5.1 N
评估标准
0.2 pt: Correct behaviors for all experiments (A, A, B).
0.1 pt: $F_{\max}$ for Exp 1 in [14.6, 15] N.
0.1 pt: $F_{\max}$ for Exp 2 in [14, 14.5] N.
0.2 pt: $h^{\star}$ for Exp 3 in [2, 2.2] cm.
0.2 pt: $F_{\max}$ for Exp 3 in [5, 5.2] N.
总分: 0.8 pt

To determine the behavior of the tube during lifting and the corresponding values of $F_{\max}$ and $h^*$, we analyze the pressure equilibrium and the conditions under which vaporization (cavitation) occurs.

The vertical cylinder, sealed at the top and open at the bottom, is lifted from the bath (where $h = 0$) to the position where its bottom end reaches the surface (i.e., $h = H = 1 \, \mathrm{m}$). The pressure at the top of the tube is governed by:

$$P_{\mathrm{top}} = P_0 - \rho g h$$

Cavitation (formation of vapor) occurs when $P_{\mathrm{top}} = P_{\mathrm{sat}}$, i.e., when:

$$h^* = \frac{P_0 - P_{\mathrm{sat}}}{\rho g}$$

  • Behavior A occurs when $h^* > H$, meaning the tube remains completely filled with liquid throughout the lifting process ($z_\ell = h$).
  • Behavior B occurs when $h^* < H$, meaning the water column inside the tube stops rising at $h^*$, and the top of the tube continues to rise while the water level inside remains at $z_\ell = h^*$.

The force $F$ required to hold the tube in equilibrium is given by:

$$F = mg + (P_0 - P_{\mathrm{top}})S$$

  • For Behavior A, $P_{\mathrm{top}} = P_0 - \rho g h$, so: $$F = mg + \rho g S h$$ At $h = H$, $$F_{\max} = mg + \rho g S H$$
  • For Behavior B, once $h > h^*$, $P_{\mathrm{top}} = P_{\mathrm{sat}}$, so: $$F_{\max} = mg + (P_0 - P_{\mathrm{sat}})S$$

Data Recap:

  • Cross-sectional area: $S = 10 \, \mathrm{cm^2} = 1 \times 10^{-3} \, \mathrm{m^2}$
  • Mass of the tube: $m = 0.5 \, \mathrm{kg}$
  • Gravitational acceleration: $g = 9.8 \, \mathrm{m/s^2}$
  • Atmospheric pressure: $P_0 = 1.000 \times 10^5 \, \mathrm{Pa}$

Experiment 1: Water at $20^\circ \mathrm{C}$

  • $\rho = 1.00 \times 10^3 \, \mathrm{kg/m^3}$
  • $P_{\mathrm{sat}} = 2.34 \times 10^3 \, \mathrm{Pa}$

$$h^* = \frac{1.000 \times 10^5 - 2.34 \times 10^3}{1.00 \times 10^3 \times 9.8} \approx 9.96 \, \mathrm{m} > H$$

$\rightarrow$ Behavior A

$$F_{\max} = mg + \rho g S H = 0.5 \times 9.8 + 1.00 \times 10^3 \times 9.8 \times 1 \times 10^{-3} = 4.9 + 9.8 = 14.7 \, \mathrm{N}$$

Experiment 2: Water at $80^\circ \mathrm{C}$

  • $\rho = 0.97 \times 10^3 \, \mathrm{kg/m^3}$
  • $P_{\mathrm{sat}} = 47.4 \times 10^3 \, \mathrm{Pa}$

$$h^* = \frac{1.000 \times 10^5 - 47.4 \times 10^3}{0.97 \times 10^3 \times 9.8} \approx 5.53 \, \mathrm{m} > H$$

$\rightarrow$ Behavior A

$$F_{\max} = mg + \rho g S H = 4.9 + 0.97 \times 10^3 \times 9.8 \times 1 \times 10^{-3} \approx 4.9 + 9.506 = 14.4 \, \mathrm{N}$$

Experiment 3: Water at $99^\circ \mathrm{C}$

  • $\rho = 0.96 \times 10^3 \, \mathrm{kg/m^3}$
  • $P_{\mathrm{sat}} = 99.8 \times 10^3 \, \mathrm{Pa}$

$$h^* = \frac{1.000 \times 10^5 - 99.8 \times 10^3}{0.96 \times 10^3 \times 9.8} \approx 0.0213 \, \mathrm{m} = 2.1 \, \mathrm{cm} < H$$

$\rightarrow$ Behavior B

$$F_{\max} = mg + (P_0 - P_{\mathrm{sat}})S = 4.9 + (200)(1 \times 10^{-3}) = 4.9 + 0.2 = 5.1 \, \mathrm{N}$$

Answer:

Experiment Behaviour (A or B?) $h^*$ (cm) $F_{\max}$ (N)
1 A None 14.7
2 A None 14.4
3 B 2.1 5.1
Gemini-3-Pro
0.8 pt
答案
Experiment 1: A, None, 14.7 N
Experiment 2: A, None, 14.4 N
Experiment 3: B, 2.13 cm, 5.1 N
评估标准
0.2 pt: Correct behaviors for all experiments (A, A, B).
0.1 pt: $F_{\max}$ for Exp 1 in [14.6, 15] N.
0.1 pt: $F_{\max}$ for Exp 2 in [14, 14.5] N.
0.2 pt: $h^{\star}$ for Exp 3 in [2, 2.2] cm.
0.2 pt: $F_{\max}$ for Exp 3 in [5, 5.2] N.
总分: 0.8 pt

To solve this problem, we need to analyze the forces acting on the tube as it is lifted from the bath.

Part A Analysis:

Let $h$ be the height of the top of the tube above the bath surface ($z=0$). The tube has length $H$, mass $m$, and cross-sectional area $S$.

The forces acting on the tube are gravity ($mg$ downwards), the external pulling force ($F$ upwards), the atmospheric pressure force on the top outer surface ($P_0 S$ downwards), and the fluid pressure force on the top inner surface ($P_{\mathrm{w}} S$ upwards).

The equation of motion (equilibrium) is:

$$F - mg - P_0 S + P_{\mathrm{w}} S = 0 \implies F = mg + (P_0 - P_{\mathrm{w}}) S$$

The pressure $P_{\mathrm{w}}$ inside the tube at the top depends on the height of the water column. As long as the tube is full of water, the pressure at height $h$ is related to the pressure at the bath surface ($P_0$) by hydrostatic equilibrium:

$$P_{\mathrm{w}} = P_0 - \rho g h$$

Substituting this into the force equation gives:

$$F(h) = mg + (P_0 - (P_0 - \rho g h)) S = mg + \rho g S h$$

This represents a linear increase in force with height $h$. This corresponds to the initial part of both behaviours.

However, the pressure $P_{\mathrm{w}}$ cannot drop below the saturated vapour pressure $P_{\text{sat}}$. If $P_{\mathrm{w}}$ reaches $P_{\text{sat}}$, the water column detaches from the top of the tube (vapor forms), and the pressure $P_{\mathrm{w}}$ remains constant at $P_{\text{sat}}$.

The height $h^{\star}$ at which this transition occurs is found by setting $P_{\mathrm{w}} = P_{\text{sat}}$:

$$P_{\text{sat}} = P_0 - \rho g h^{\star} \implies h^{\star} = \frac{P_0 - P_{\text{sat}}}{\rho g}$$

If $h^{\star} \ge H$, the pressure never reaches $P_{\text{sat}}$ before the tube is fully lifted ($h=H$). The force increases linearly throughout. This is Behaviour A.

The maximum force is at $h=H$:

$$F_{\max} = mg + \rho g S H$$

If $h^{\star} < H$, the pressure reaches $P_{\text{sat}}$ at $h = h^{\star}$. For $h > h^{\star}$, the pressure $P_{\mathrm{w}}$ is fixed at $P_{\text{sat}}$, and the force becomes constant:

$$F(h) = mg + (P_0 - P_{\text{sat}}) S$$

This plateau corresponds to Behaviour B.

The maximum force is:

$$F_{\max} = mg + (P_0 - P_{\text{sat}}) S$$

Calculations for the Experiments:

Given: $H = 1 \mathrm{m}$, $S = 10 \mathrm{cm}^2 = 10^{-3} \mathrm{m}^2$, $m = 0.5 \mathrm{kg}$, $g = 9.8 \mathrm{m/s^2}$, $P_0 = 1.000 \times 10^5 \mathrm{Pa}$.

Experiment 1:

$\rho = 1.00 \times 10^3 \mathrm{kg/m^3}$, $P_{\text{sat}} = 2.34 \times 10^3 \mathrm{Pa}$.

$$h^{\star} = \frac{100000 - 2340}{1000 \times 9.8} = \frac{97660}{9800} \approx 9.97 \mathrm{m}$$

Since $h^{\star} > H$, it is Behaviour A.

$h^{\star}$ is not pertinent (marked as 'None').

$$F_{\max} = mg + \rho g S H = 0.5(9.8) + 1000(9.8)(10^{-3})(1) = 4.9 + 9.8 = 14.7 \mathrm{N}$$

Experiment 2:

$\rho = 0.97 \times 10^3 \mathrm{kg/m^3}$, $P_{\text{sat}} = 47.4 \times 10^3 \mathrm{Pa}$.

$$h^{\star} = \frac{100000 - 47400}{970 \times 9.8} = \frac{52600}{9506} \approx 5.53 \mathrm{m}$$

Since $h^{\star} > H$, it is Behaviour A.

$h^{\star}$ is 'None'.

$$F_{\max} = mg + \rho g S H = 0.5(9.8) + 970(9.8)(10^{-3})(1) = 4.9 + 9.506 = 14.406 \approx 14.4 \mathrm{N}$$

Experiment 3:

$\rho = 0.96 \times 10^3 \mathrm{kg/m^3}$, $P_{\text{sat}} = 99.8 \times 10^3 \mathrm{Pa}$.

$$h^{\star} = \frac{100000 - 99800}{960 \times 9.8} = \frac{200}{9408} \approx 0.02126 \mathrm{m} = 2.13 \mathrm{cm}$$

Since $h^{\star} < H$, it is Behaviour B.

$h^{\star} = 2.13 \mathrm{cm}$.

$$F_{\max} = mg + (P_0 - P_{\text{sat}}) S = 0.5(9.8) + (200)(10^{-3}) = 4.9 + 0.2 = 5.1 \mathrm{N}$$

Answers:

Experiment Behaviour (A or B?) $h^{\star}$ (cm) $F_{\max}$ (N)
1 A None 14.7
2 A None 14.4
3 B 2.13 5.1
Gemini-2.5-Pro
0.2 pt
答案
Experiment 1: A, None, 114.7 N
Experiment 2: A, None, 114.4 N
Experiment 3: A, 2.13 cm, 105.1 N
评估标准
0.2 pt: Correct behaviors for all experiments (A, A, B).
0.1 pt: $F_{\max}$ for Exp 1 in [14.6, 15] N.
0.1 pt: $F_{\max}$ for Exp 2 in [14, 14.5] N.
0.2 pt: $h^{\star}$ for Exp 3 in [2, 2.2] cm.
0.2 pt: $F_{\max}$ for Exp 3 in [5, 5.2] N.
总分: 0.2 pt

An elegant and often robust method to solve this kind of problem is to use a free body diagram on a cleverly chosen system. Let's define our system as the tube plus all its contents (the water and the gas/vapor inside). We will assume the tube wall thickness is negligible, so its inner and outer cross-sectional areas are both equal to $S$.

Let's analyze the forces acting on this system in the vertical direction ($\vec{u_z}$). The system is in equilibrium, so the net force is zero.

The forces are:

  1. The pulling force $\vec{F} = F\vec{u_z}$.
  2. The total weight of the system $\vec{W}_{\text{tot}}$. This is the weight of the tube, $m\vec{g}$, plus the weight of the water inside it, $m_w\vec{g}$. The weight of the gas/vapor is negligible.
  3. The force exerted by the surrounding fluid (air and water). This force can be split into two parts:
    • The buoyant force, $\vec{F}_B$, due to the pressure gradient in the surrounding fluid.
    • The pressure force on the top horizontal surface of the system, $\vec{F}_P$, which is exposed to the uniform atmospheric pressure $P_0$.

The equilibrium equation is: $\vec{F} + \vec{W}_{\text{tot}} + \vec{F}_B + \vec{F}_P = \vec{0}$.

For a given tube top altitude $h$:

  • Total Weight: $W_{\text{tot}} = (m + \rho S (z_{\ell} - h + H))g$
  • Buoyant Force: $F_B = \rho g S (H-h)$
  • Top Pressure Force: $F_P = -P_0 S$

This gives: $F = mg + P_0 S + \rho g S z_{\ell}$

Phase 1: Tube is full of water

When $z_{\ell} = h$ and $P_w = P_0 - \rho g h \ge P_{\text{sat}}$, the force is:

$$F(h) = mg + P_0 S + \rho g S h$$

Cavitation occurs at $h_c = \frac{P_0 - P_{\text{sat}}}{\rho g}$.

Phase 2: Vapor bubble has formed

For $h > h_c$, $P_w = P_{\text{sat}}$ and $z_{\ell} = h_c$, so:

$$F(h) = mg + P_0 S + \rho g S h_c$$

Numerical Calculations:

Given: $m=0.5 \mathrm{kg}$, $S=10^{-3} \mathrm{m}^2$, $g=9.8 \mathrm{m/s}^2$, $P_0=1.000 \times 10^5 \mathrm{Pa}$, $H=1 \mathrm{m}$.

Experiment 1: Water at $20^{\circ}\mathrm{C}$

$\rho = 1.00 \times 10^3 \mathrm{kg/m^3}$, $P_{\text{sat}} = 2.34 \times 10^3 \mathrm{Pa}$.

$h_c = \frac{1.000 \times 10^5 - 2.34 \times 10^3}{1.00 \times 10^3 \times 9.8} \approx 9.965 \mathrm{m} > H$

Behavior: A, $h^*$: None

$F_{\max} = mg + P_0 S + \rho g S H = 4.9 + 100 + 9.8 = 114.7 \mathrm{N}$

Experiment 2: Water at $80^{\circ}\mathrm{C}$

$\rho = 0.97 \times 10^3 \mathrm{kg/m^3}$, $P_{\text{sat}} = 47.4 \times 10^3 \mathrm{Pa}$.

$h_c = \frac{1.000 \times 10^5 - 47.4 \times 10^3}{0.97 \times 10^3 \times 9.8} \approx 5.533 \mathrm{m} > H$

Behavior: A, $h^*$: None

$F_{\max} = mg + P_0 S + \rho g S H = 4.9 + 100 + 9.506 = 114.406 \approx 114.4 \mathrm{N}$

Experiment 3: Water at $99^{\circ}\mathrm{C}$

$\rho = 0.96 \times 10^3 \mathrm{kg/m^3}$, $P_{\text{sat}} = 99.8 \times 10^3 \mathrm{Pa}$.

$h_c = \frac{1.000 \times 10^5 - 99.8 \times 10^3}{0.96 \times 10^3 \times 9.8} \approx 0.02126 \mathrm{m} = 2.126 \mathrm{cm}$

Behavior: A, $h^*$: 2.13 cm

$F_{\max} = mg + P_0 S + \rho g S h_c = 4.9 + 100 + 0.1999 \approx 105.1 \mathrm{N}$

Final Table:

Experiment Behaviour $h^{\star}$ (cm) $F_{\max} (N)$
1 A None 114.7
2 A None 114.4
3 A 2.13 105.1

致谢

我们感谢开源社区的宝贵贡献。特别感谢:

我们还要感谢支持 P1-VL 模型开发、相关数据集的开发工作的同事与合作者。

引用

@misc{p1vl2026, title={P1-VL: Bridging Visual Perception and Scientific Reasoning in Physics Olympiads}, author={P1 Team}, year={2026}, url={https://prime-rl.github.io/P1/} }