IPhO 2025, Теория — Задача 1. Hydrogen and galaxies
Theory — Q1 — Hydrogen and galaxies (10 points) · 10 т.
Условие
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.
Throughout this problem we will only use , defined as .
Part A - Introduction
Bohr model
We assume that the hydrogen atom consists of a non-relativistic electron, with mass , orbiting a fixed proton. Throughout this part, we assume its motion is on a circular orbit.
In the Bohr model, we assume the magnitude of the electron's angular momentum is quantized, where is an integer. We define .
Hydrogen fine and hyperfine structures
The rare spontaneous inversion of the electron's spin causes a photon to be emitted on average once per 10 million years per hydrogen atom. This emission serves as a hydrogen tracer in the universe and is thus fundamental in astrophysics. We will study the transition responsible for this emission in two steps.
First, consider the interaction between the electron spin and the relative motion of the electron and the proton. Working in the electron's frame of reference, the proton orbits the electron at a distance . This produces a magnetic field .
Second, the electron spin creates a magnetic moment . Its magnitude is roughly . The fine (F) structure is related to the energy difference between an electron with a magnetic moment parallel to and that of an electron with anti-parallel to . Similarly, the hyperfine (HF) structure is related to the energy difference , due to the interaction between parallel and anti-parallel magnetic moments of the electron and the proton. It is known to be approximately where is the proton mass.
Part B - Rotation curves of galaxies
Data
- Kiloparsec:
- Solar mass :
We consider a spherical galaxy centered around a fixed point . At any point , let be the volumetric mass density and the associated gravitational potential (i.e. potential energy per unit mass). Both and depend only on . The motion of a mass located at , due to the field , is restricted to a plane containing .
Fig. 1(A) is a picture of the spiral galaxy NGC 6946 in the visible band (from the 0.8 m Schulman Telescope at the Mount Lemmon Sky Center in Arizona). The little ellipses in Fig. 1(B) show experimental measurements of for this galaxy. The central region () is named the bulge. In this region, the mass distribution is roughly homogeneous. The red curve is a prediction for if the system were homogeneous in the bulge and keplerian ( with ) outside it, i.e. considering that the total mass of the galaxy is concentrated in the bulge.
![(A) Visible-band photograph of the spiral galaxy NGC 6946 with a scale bar of 18 kpc; (B) rotation curve plot with experimental points (small ellipses) and a red keplerian-model curve; vertical axis $v_c$ [km/s] from 0 to 200, horizontal axis $r$ [kpc] from 0 to 10.](https://pub-43290baaaff14857b5dd59610ea438c7.r2.dev/problems/ipho-2025-theory-q1/p1-fig1.png)
Comparing the keplerian model and the experimental data makes astronomers confident that part of the mass is invisible in the picture. They thus suppose that the galaxy's actual mass density is given by
where and are constants.
Part C - Mass distribution in our galaxy
For a spiral galaxy, the model for Eq. 1 is modified and one usually considers the gravitational potential is given by , where is the distance to the galactic plane (defined by ), and is now the axial radius and a constant to be determined. and are constant values.
From here on, we set .
Therefore, outside the bulge the velocity modulus does not depend on the distance to the galactic center. We will use this fact, as astronomers do, to measure the galaxy's mass distribution from the inside.
All galactic objects considered here for astronomical observations, such as stars or nebulae, are primarily composed of hydrogen. Outside the bulge, we assume that they rotate on circular orbits around the galactic center . is the sun's position and that of a given galactic object emitting in the hydrogen spectrum. In the galactic plane, we consider a line of sight corresponding to the orientation of an observation, on the unit vector (see Fig. 2).

Let be the galactic longitude, measuring the angle between and the . The sun's velocity on its circular orbit of radius is denoted . A galactic object in orbits on another circle of radius at velocity . Using a Doppler effect on the previously studied 21 cm line, one can obtain the relative radial velocity of the emitter with respect to the sun : it is the projection of on the line of sight.
Using a radio telescope, we make observations in the plane of our galaxy toward a longitude . The frequency band used contains the 21 cm line, whose frequency is . The results are reported in Fig. 3.

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 as a function of the measured total mass of each galaxy gives an interesting correlation called the Tully-Fischer relation, see Fig. 4 (right).

In the extremely low acceleration regime, of the order of , the MOdified Newtonian Dynamics (MOND) theory suggests that one can modify Newton's second law using where is the modulus of the acceleration and the function is defined by .
A.1 Determine the electron's velocity in a circular orbit of radius . [0,2 т.]
A.2 Show that the radius of each orbit is given by , where is called the Bohr radius. Express in terms of , , and and calculate its numerical value with 3 digits. Express , the velocity on the orbit of radius , in terms of and . [0,5 т.]
A.3 Determine the electron's mechanical energy on an orbit of radius in terms of , , and . Determine in the ground state in terms of , and . Compute its numerical value in eV. [0,5 т.]
A.4 Determine the magnitude of at the position of the electron in terms of , , , and . [0,5 т.]
A.5 Express as a function of and .
Express the wavelength of a photon emitted during a transition between the two states of the hyperfine structure and give its numerical value with two digits. [0,5 т.]
B.1 In the case of a circular orbit, determine the velocity of an object on a circular orbit passing through in terms of and . [0,2 т.]
B.2 Deduce the mass of the bulge of NGC 6946 from the red rotation curve in Fig. 1(B), in solar mass units. [0,5 т.]
B.3 Show that the velocity profile , corresponding to the mass density in Eq. 1, can be written . Express and in terms of , and .
( Hints: , and: for . )
Simplify when and when .
Show that if , the mass embedded in a sphere of radius with the mass density given by Eq. 1 simplifies and depends only on and .
Estimate the mass of the galaxy NGC 6946 actually present in the picture in Fig. 1(A). [1,8 т.]
C.1 Find the equation of motion on for the vertical motion of a point mass in such a potential, assuming is constant. Show that, if , the galactic plane is a stable equilibrium state by giving the angular frequency of small oscillations around it. [0,5 т.]
C.2 Identify the regime, either or , in which the model of Eq. 1 recovers a potential of the form with a suitable definition of .
Under this condition no longer depends on . Express it in terms of . [0,6 т.]
C.3 Determine in terms of , , and . Then, express in terms of , , and . [0,7 т.]
C.4 In our galaxy, . Determine the values of the relative radial velocity (with 3 significant digits) and the distance from the galactic center (with 2 significant digits) of the 3 sources observed in Fig. 3. Distances should be expressed as multiples of . [0,6 т.]
C.5 On the top view of our galaxy (in the answer box), indicate the positions of the sources observed in Fig. 3.
What could be deduced from repeated measurements changing ? [0,6 т.]
D.1 Assuming that the radius of a galaxy doesn't depend on its mass, show that the model of Eq. 1 (part B) gives a relation of the form where and should be specified.
Compare this expression to the Tully-Fischer relation by computing . [0,4 т.]
D.2 Using data for NGC 6946 in Fig. 1, estimate, within Newton's theory, the modulus of the acceleration of a mass in the outer regions of NGC 6946. [0,2 т.]
D.3 Let be a mass on a circular orbit of radius with velocity in the gravity field of a fixed mass .
Within the MOND theory, with , determine the Tully-Fischer exponent.
Using data for NGC 6946 and/or Tully-Fischer law, calculate to show that MOND operates in the correct regime. [0,8 т.]
D.4 Considering relevant cases, determine for all values of in the MOND theory in the case of a gravitational field due to a homogeneously distributed mass with radius . [0,9 т.]
Решение
Part A - Introduction
Bohr model
A.1
SOLUTION:
Newton's second law on the electron in the electrical field of the proton for a circular orbit and projected on : hence
Marking Scheme
| A.1.1 : Using Newton's second law | 0.1 |
|---|---|
| A.1.2 : Expression of the velocity | 0.1 |
In the Bohr model, we assume the magnitude of the electron's angular momentum is quantized, where is an integer. We define .
A.2
SOLUTION:
If the norm of the angular momentum is quantified, for a circular orbit of radius it is . In the previous question, we have already obtained a relation between and that can be used for and and gives . Then using the quantified expression we get thus and then . For the numerical value we previously compute and then . For the velocity, we get and then .
Marker Scheme
| A.2.1 : Expression of | 0.1 |
|---|---|
| A.2.2 : Expression of | 0.1 |
| A.2.3 : Numerical value for | 0.1 |
| A.2.4 : Expression of | 0.2 |
A.3
SOLUTION:
The mechanical energy is , hence then for the ground state . Using the expression of , we get the beautiful formula . The numerical value is which corresponds to .
Marker Scheme
| A.3.1 : Expression for | 0.2 |
|---|---|
| A.3.2 : Expression for with | 0.2 |
| A.3.3 : Numerical value for | 0.1 |
Hydrogen fine and hyperfine structures
The rare spontaneous inversion of the electron's spin causes a photon to be emitted on average once per 10 million years per hydrogen atom. This emission serves as a hydrogen tracer in the universe and is thus fundamental in astrophysics. We will study the transition responsible for this emission in two steps.
First, consider the interaction between the electron spin and the relative motion of the electron and the proton. Working in the electron's frame of reference, the proton orbits the electron at a distance . This produces a magnetic field .
A.4
SOLUTION:
The period of the motion is : .
The current corresponding to the orbit of the proton is hence .
The magnetic field created by a loop with current and radius is : , which here gives .
Marker Scheme
| A.4.1 : Expression for the period | 0.1 |
|---|---|
| A.4.2 : Expression for the current | 0.2 |
| A.4.3 : General expression for | 0.1 |
| A.4.4 : Inject into | 0.1 |
Second, the electron spin creates a magnetic moment . Its magnitude is roughly . The fine (F) structure is related to the energy difference between an electron with a magnetic moment parallel to and that of an electron with anti-parallel to . Similarly, the hyperfine (HF) structure is related to the energy difference , due to the interaction between parallel and anti-parallel magnetic moments of the electron and the proton. It is known to be approximately where is the proton mass.
A.5
SOLUTION:
The potential energy corresponding to the interaction between the spin magnetic moment and the nuclear magnetic field :
The difference between the energy of two electrons with a spin parallel and antiparallel to is then . Using previous expressions one finds: which writes hence .
The wavelength of the photon corresponding to this transition is then hence whose value is .
Marker Sheme
| A.5.1 : Expression for the potential energy | 0.1 |
|---|---|
| A.5.2 : Expression for | 0.1 |
| A.5.3 : Expression for in term of | 0.1 |
| A.5.4 : Expression for | 0.1 |
| A.5.5 : Numerical value for | 0.1 |
Part B - Rotation curves of galaxies
Data
- Kiloparsec:
- Solar mass :
We consider a spherical galaxy centered around a fixed point . At any point , let be the volumetric mass density and the associated gravitational potential (i.e. potential energy per unit mass). Both and depend only on . The motion of a mass located at , due to the field , is restricted to a plane containing .
B.1
SOLUTION:
The force created by the potential is . Newton's second law for a circular orbit then gives hence .
SOLUTION:
| B.1.1 : Using Newton's second law | 0.1 |
|---|---|
| B.1.2 : Expression for the velocity. | 0.1 |
[[фигура p1-sol-fig1]]
Fig. 1(A) is a picture of the spiral galaxy NGC 6946 in the visible band (from the 0.8m Schulman Telescope at the Mount Lemmon Sky Center in Arizona). The little ellipses in Fig. 1(B) show experimental measurements of for this galaxy. The central region () is named the bulge. In this region, the mass distribution is roughly homogeneous. The red curve is a prediction for if the system were homogeneous in the bulge and keplerian ( with ) outside it, i.e. considering that the total mass of the galaxy is concentrated in the bulge.

B.2
SOLUTION:
Either by Gauss's theorem , then one gets . or one knows the law and intuits that one can use the interior mass
If there is almost no more mass after the bulge radius
then if , and . But .
This gives .
One can then deduce that if the velocity is given only by the bulge, at a given distance we must have . On the red curve we can read at hence so that .
Marker Scheme
| B.2.1 : via Gauss' Theorem or another method resulting in an equivalent result. | 0.1 |
|---|---|
| B.2.2 : Expression for | 0.1 |
| B.2.3 : Expression for | 0.1 |
| B.2.4 : Taking the right value of in the figure | 0.1 |
| B.2.5 : Numerical value for with a tolerance of | 0.1 |
Comparing the keplerian model and the experimental data makes astronomers confident that part of the mass is invisible in the picture. They thus suppose that the galaxy's actual mass density is given by
where and are constants.
B.3
SOLUTION:
On the one hand, writing Gauss' theorem on a sphere of radius gives and thus . As long as this final formula is given it doesn't matter the method.
But, on the other hand hence
But as we finally get wich writes
One can then read and
Two regime could be considered:
- if , a third order Taylor expansion of gives ,
- and if then and .
The function is vanishing when and is asymptotically constant with value when : this corresponds to the observational curve for the galaxy considered (black circles on the right part of figure 1(B). A natural interpretation for is the typical radius beyond which the circular velocity is constant. On this picture one can read for the constant value of after , then one can deduce . The mass embedded in a sphere of radius is given by which reduces to if . In the picture we have a radius of the galaxy, then a mass . This mass corresponds to more than ten times the value of the mass actually visible in this picture : this is the dark matter concept.
Marker Scheme
| B.3.1 : via Gauss' Theorem or another method resulting in an equivalent result. | 0.2 |
|---|---|
| B.3.2 : Interior mass | 0.3 |
| B.3.3. : Expression for | 0.1 |
| B.3.4 : Using Newton's second law | 0.1 |
| B.3.5 : Expression for | 0.1 |
| B.3.6 : Expression for | 0.1 |
| B.3.7 : Simplification for in the case | 0.2 |
| B.3.8 : Simplification for in the case | 0.2 |
| B.3.9 : Value of | 0.2 |
| B.3.10 : Expression for in the case | 0.2 |
| B.3.11 : Mass in the figure (good if nearest power of ten) | 0.1 |
Part C - Mass distribution in our galaxy
For a spiral galaxy, the model for Eq. 1 is modified and one usually considers the gravitational potential is given by , where is the distance to the galactic plane (defined by ), and is now the axial radius and a constant to be determined. and are constant values.
C.1 — Find the equation of motion on for the vertical motion of a point mass in such a potential, assuming is constant. Show that, if , the galactic plane is a stable equilibrium state by giving the angular frequency of small oscillations around it. [0.5pt]
SOLUTION:
The equation of motion is given by Newton's second law , projected on , it gives . Using the given potential we have . Near the galactic plane ( ) the exponential is equal to 1 and can be simplified to give . If the ln is negative and the equation of motion is of the form with . This proves that is oscillating around and that the motion is stable.
Marker Scheme
| C.1.1 : Newton's second law, or equivalent method | 0.1 |
|---|---|
| C.1.2 : Projection on the z axis | 0.1 |
| C.1.3 : Equation of motion | 0.1 |
| C.1.4 : Equation near the galactic plane | 0.1 |
| C.1.5 : Expression for | 0.1 |
From here on, we set .
C.2 — Identify the regime, either or , in which the model of Eq. 1 recovers a potential of the form with a suitable definition of . Under this condition no longer depends on . Express it in terms of . [0.6pt]
SOLUTION:
Using the density given by equation (1) in part B, we have obtained
Hence, considering , one can simplify this relation to . The gravitational potential can be obtained by integration, we then have : . The constant can be found by correctly choosing the origin of the potential. This potential corresponds to: with . In that case, the equation of motion in the galactic plane gives which writes , so that .
Marker Scheme
| C2.1 : Condition for simplication | 0.1 |
|---|---|
| C2.2 : Expression for | 0.2 |
| C2.3 : Identification of | 0.1 |
| C2.4 : Newton's second law | 0.1 |
| C2.5 : Expression for | 0.1 |
Therefore, outside the bulge the velocity modulus does not depend on the distance to the galactic center. We will use this fact, as astronomers do, to measure the galaxy's mass distribution from the inside.
All galactic objects considered here for astronomical observations, such as stars or nebulae, are primarily composed of hydrogen. Outside the bulge, we assume that they rotate on circular orbits around the galactic center . is the sun's position and that of a given galactic object emitting in the hydrogen spectrum. In the galactic plane, we consider a line of sight corresponding to the orientation of an observation, on the unit vector (see Fig. 2).

[[фигура p1-sol-fig4]]
Fig. 2: Geometry of the measurement
Let be the galactic longitude, measuring the angle between and the . The sun's velocity on its circular orbit of radius is denoted . A galactic object in orbits on another circle of radius at velocity . Using a Doppler effect on the previously studied 21 cm line, one can obtain the relative radial velocity of the emitter with respect to the sun : it is the projection of on the line of sight.
C.3 — Determine in terms of , , and . Then, express in terms of , , and . [0.7pt]
SOLUTION:
We have and . In the right triangle the sum of angles gives , but, as is perpendicular to the radius , we also have : then . On the other side, we have , which gives . Merging all of these results and taking into account that and that we have and finally .
Marker Scheme
| C3.1 : Expression for | 0.1 |
|---|---|
| C3.2 : Expression for | 0.1 |
| C3.3 : | 0.1 |
| C3.4 : Expression for | 0.1 |
| C3.5 : Expression for | 0.2 |
| C3.6 : Expression for | 0.1 |
Using a radio telescope, we make observations in the plane of our galaxy toward a longitude . The frequency band used contains the 21 cm line, whose frequency is . The results are reported in Fig. 3.

[[фигура p1-sol-fig2]]
Fig. 3: Electromagnetic signal as a function of the frequency shift, measured in the radio frequency band at using EU-HOU RadioAstronomy
C.4 — In our galaxy, . Determine the values of the relative radial velocity (with 3 significant digits) and the distance from the galactic center (with 2 significant digits) of the 3 sources observed in Fig. 3. Distances should be expressed as multiples of . [0.6pt]
SOLUTION:
In Fig. 3 one can measure the 3 frequency shifts ( ) corresponding to each peak : , and . One can then compute the relative Doppler velocity using , with one gets
As peaks are placed on grid points, the tolerance in the value is due to fact that candidates could use in the place of the 9 digits given in the formulary.
The corresponding distances from the galactic center are then obtained using the relation , with we obtain :
Marker Scheme
| C4.1 : Doppler formula for | 0.1 |
|---|---|
| C4.2 : Getting the 3 numerical values for | 0.2 |
| C4.3 : Numerical values of the 3 velocities () | 0.2 |
| C4.4 : Numerical values of the 3 distances () | 0.1 |
C.5 — On the top view of our galaxy (in the answer box), indicate the positions of the sources observed in Fig. 3. What could be deduced from repeated measurements changing ? [0.6pt]
SOLUTION:
As indicated on the figure below, the right line of sight could be obtained geometrically (i.e. without protractor) : using the 15° grid graduation one can going back from 30° from the perpendicular line to CS, we then obtain a radius which perpendicular to the line of sight, in other words as the line of sight is passing by S and is tangenting the circle of radius CS/2.
Drawing the circles or radius , and , the line of sight with from we get 2 possible intersection for each peak : a near one and a far one. We plot only the nearest for each source on the answer figure.
[[фигура p1-sol-fig3]]

The far intersections for each source is much further away and hence is likely less intense. Astronomers could also use the variation in the radio signal when they slowly vary the longitude to determine the right position of the actual source. A continuous variation of in the interval makes hydrogen sources appear in the galaxy, as the galaxy is essentially composed of hydrogen, one can trace its mass distribution : i.e. the spiral structure.
Marker Scheme
| C5.1 : Getting the right line of sight | 0.1 |
|---|---|
| C5.2 : Drawing for the 3 circles | 0.2 |
| C5.3 : Drawing for the 3 points | 0.2 |
| C5.4 : Deduction | 0.1 |
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 as a function of the measured total mass of each galaxy gives an interesting correlation called the Tully-Fischer relation, see Fig. 4 (right).
[[фигура p1-sol-fig5]]

Fig. 4. Left: Rotation curves for typical spiral galaxies - Right: as a function of on linear scales. Colored dots correspond to different galaxies and different surveys. The green line is the Tully-Fischer relation which is in very good agreement with the best fit line of the data (in black).
D.1 — SOLUTION:
We have obtained and for a galaxy of radius , we have . This gives and . This relation is of the expected form with and . Analysing the data we get the power law exponent of the Tully-Fisher relation as : the dark matter model from part B is not able to reproduce this law.
Marker Scheme
| D1.1 : Recall for | 0.1 |
|---|---|
| D1.2 : Expression for | 0.1 |
| D1.3 : Expression for | 0.1 |
| D1.4 : Numerical value for (correct if it is between 3.5 and 4) | 0.1 |
In the extremely low acceleration regime, of the order of , the MOdified Newtonian Dynamics (MOND) theory suggests that one can modify Newton's second law using where is the modulus of the acceleration and the function is defined by .
D.2 — SOLUTION:
Considering that outer orbits are circular, the corresponding acceleration for a test mass is radial and given in newtonian theory by . In the case of NGC 6946, the value of the velocity is roughly constant and equal to as far . For this smallest distance from the center, the acceleration is , this value is the maximal acceleration to which as star is submitted in the outer regions of this galaxy. It corresponds to the MOND regime.
Marker Scheme
| D2.1 : Expression for | 0.1 |
|---|---|
| D2.2 : Numerical value for (good nearest power of ten) | 0.1 |
D.3 — SOLUTION:
If , then and MOND theory gives . Considering a gravitational interaction between and we then have for the radial component of the modified Newton's second Law . The radial acceleration on a circular orbit of radius is always given by , the modified second law writes now which gives , and thus . Considering the notation from D.1, this is a power law relation with in accordance with the Tully-Fischer relation.
For the NGC 6946 galaxy, we read thus and one can read the corresponding total mass by the Tully-Fischer relation as thus . One can obtain similar numbers using experimental data on the curve of Fig. 4. Introducing these values in the relation it gives as expected.
Marker Scheme
| D3.1 : Considering the hypothesis | 0.1 |
|---|---|
| D3.2 : Newton's second law | 0.1 |
| D3.3 : Expression for | 0.1 |
| D3.4 : Numerical value for | 0.1 |
| D3.5 : Numerical value for | 0.1 |
| D3.6 : Numerical value for | 0.1 |
| D3.7 : Expression for | 0.1 |
| D3.8 : Numerical value for (good if nearest power of ten) | 0.1 |
D.4 — SOLUTION:
Taking the full formula for , the modified second law with circular velocity at radius writes now where is the gravitational field of the homogeneous ball of mass and with radius . This field can be deduced from Gauss' theorem it is
Outside the ball : . After a small reorganisation, appears to be solution of the biquadratic equation . The positive root of this equation is
When , is asymptotically constant and which is the Tully-Fisher relation. Inside the ball : . With a similar reorganisation, appears now to be solution of another biquadratic equation which is . The positive solution is now
When , we recover as in the experimental data.
Marker Scheme
| D4.1 : Modified second law | 0.1 |
|---|---|
| D4.2 : Gravitational field in the case | 0.1 |
| D4.3 : Gravitational field in the case | 0.1 |
| D4.4 : Bi-quadratic equation in the case | 0.1 |
| D4.5 : Expression for in the case | 0.1 |
| D4.6 : Behaviour in the limit | 0.1 |
| D4.7 : Bi-quadractic equation for | 0.1 |
| D4.8 : Expression for when | 0.1 |
| D4.9 : Behaviour when | 0.1 |
Оригинал в Архива: IPhO_2025_Q1.pdf · официални решения: IPhO_2025_S1.pdf