IOM 2017, Теория — Задача 3. Neutrino

The 2nd International Olympiad of Metropolises — physics, theoretical part, 2017 · 40 т.

Внимание: Бележка към темата

Three whole native tasks with ten connected requests each. The archived radiography key contains two full proposed solutions with different flash/wavelength/angle values and scores35/20; both are retained, and question2/paper total points are unspecified. Printed equations, mass ranges, signs and notation defects remain literal with separate archive source notes.

Native source header and key scope

The 2nd International Olympiad of Metropolisesphysics — theoretical part — 2017.

The native question edition contains three problems: CARBONATED WATER, RADIOGRAPHY and Neutrino, each with ten connected numbered requests. Neutrino has three native titled parts. The original header has the concatenated word “Metropolisesphysics”. No examination date, time limit or whole-paper score is printed in this question packet.

The retained matching archived key repeats the questions, supplies full proposed solutions and grading tables, and contains two distinct complete radiography key variants. Carbonated water is graded25, radiography35 in the first table and20 in the second, and Neutrino40. Neither radiography table is designated as the sole scoring authority in these retained sources. Key pages16 and27 are blank. All38 original pages remain retained; the keys are labelled as archive solutions.

Условие

Neutrino is one of the most peculiar elementary particles. It has no electric charge and does not participate in the strong interactions (which are responsible for stability of atomic nuclei). Physicists use the word «flavor» to specify a neutrino type. There are three neutrino flavors known to date: electron neutrino νe\nu_e, muon neutrino νμ\nu_\mu, and tau-neutrino ντ\nu_\tau. A neutrino of each flavor has its antiparticle (antineutrino). The symbols used for the latter are the same as for neutrinos but with an upper bar: νˉe\bar\nu_e, νˉμ\bar\nu_\mu, and νˉτ\bar\nu_\tau.

Neutrino participates only in the weak interactions, the most famous process mediated by the weak interaction is β\beta-decay. In this process a single neutron in atomic nucleus decays into a proton, an electron, and an electron antineutrino: n→p+e+νˉen\to p+e+\bar\nu_e (however, it would be a mistake to think than neutron is composed of these particles, there is also a process p→n+e++νep\to n+e^++\nu_e!).

A neutrino is always created together with its antineutrino or a charged antilepton (positron e+e^+ (an electron antiparticle), antimuon μ+\mu^+, or antitau-lepton τ+\tau^+). An antineutrino, in turn, is always created together with its neutrino or the corresponding charged lepton.

Neutrinos are extremely lightweight, their masses are several orders of magnitude less than masses of other matter particles. The precise values of neutrino masses are still unknown. Due to their small masses all neutrinos participating in nuclear reactions are ultrarelativistic, i.e. their velocities are very close to the speed of light in vacuum. The energy of such a neutrino of mass mm and momentum p⃗\vec p is almost independent of its mass:

E=m2c4+c2p⃗ 2≈c∣p⃗∣.E=\sqrt{m^2c^4+c^2\vec p^{\,2}}\approx c|\vec p|.

A neutrino, like many other elementary particles, has spin, i.e. the proper angular momentum, which is non-zero even in the neutrino rest frame. A specific feature of all detected neutrinos (antineutrinos) is the negative (positive) sign of its spin component projected on the direction of neutrino (antineutrino) momentum. Loosely speaking, a neutrino does not have a «mirror reflection». Other elementary matter particles can have both signs of the spin component. Physicists explain this fact by saying that neutrinos with other spin component either do not exist, or do not participate even in the weak interactions (so they cannot be detected).

Physical constants and data (can be used in any part of the problem)

  • speed of light in vacuum c≈3⋅108 m/sc\approx3\cdot10^8\ \mathrm{m/s};
  • gravitational constant G≈6,7⋅10−11 m3/(kg⋅s2)G\approx6{,}7\cdot10^{-11}\ \mathrm{m^3/(kg\cdot s^2)};
  • Planck constant ℏ≈10−34 J⋅s\hbar\approx10^{-34}\ \mathrm{J\cdot s};
  • proton radius rp≈10−15 mr_p\approx10^{-15}\ \mathrm m;
  • Avogadro constant NA≈6⋅1023 mole−1N_A\approx6\cdot10^{23}\ \mathrm{mole^{-1}};
  • hydrogen molar mass μ≈2 g/mole\mu\approx2\ \mathrm{g/mole};
  • Solar mass MC≈2⋅1030 kgM_C\approx2\cdot10^{30}\ \mathrm{kg};
  • Solar radius rC≈7⋅108 mr_C\approx7\cdot10^8\ \mathrm m;
  • mean radius of Earth’s orbit a≈1,5⋅1011 ma\approx1{,}5\cdot10^{11}\ \mathrm m;
  • eccentricity of Earth’s orbit ε≈0,017\varepsilon\approx0{,}017;
  • radius of «active» solar core where nuclear fusion proceeds and neutrinos are created ra≈1,2⋅108 mr_a\approx1{,}2\cdot10^8\ \mathrm m;
  • range of electron density nen_e inside the Sun from the active core to outer layers: from 5,9⋅1031 m−35{,}9\cdot10^{31}\ \mathrm{m^{-3}} to 1029 m−310^{29}\ \mathrm{m^{-3}};
  • parsec (pc), an astronomical unit of length, 1 pc≈3,2 light year≈3⋅1016 m1\ \mathrm{pc}\approx3{,}2\ \text{light year}\approx3\cdot10^{16}\ \mathrm m.
  • electronvolt (eV) is the unit of energy equal to the work done by electrostatic force moving a single electron across potential difference of 1 V.

Part I: neutrino masses and oscillations.

The Nobel Prize of 2015 was awarded for the «discovery of neutrino oscillations indicating that neutrinos are massive». Neutrino oscillations is a process of interconversion of neutrino flavors. According to modern theoretical models the possibility of neutrino oscillations is indeed closely related to their masses (massless neutrinos cannot oscillate).

It should be noted that neutrinos like other elementary particles are not some «immutable» entities, rather they are quanta of a neutrino field (similarly to photons which are quanta of electromagnetic field). Therefore, in different physical situations they can appear in the states with different properties. For instance, neutrino state of a certain flavor (a state in which neutrino is created or annihilated in nuclear reactions) does not coincide with neutrino state of a certain mass.

To be specific, consider oscillation νe↔νμ\nu_e\leftrightarrow\nu_\mu (i.e. we neglect the third neutrino flavor). An intensive flow of neutrinos can be regarded as «almost classical» radiation of a given wavelength (here the analogy with electromagnetic wave, an «almost classical» flow of a large number of photons, applies again).

The existence of several neutrino states can be described by introducing a «polarization»:

u⃗(t,r⃗)=u⃗1cos⁡(ω1t−k⃗r⃗)+u⃗2cos⁡(ω2t−k⃗r⃗).\vec u(t,\vec r)=\vec u_1\cos(\omega_1t-\vec k\vec r)+\vec u_2\cos(\omega_2t-\vec k\vec r).

The quotation mark indicates that this polarization is not a polarization in the «regular» space, this is polarization in the «space of neutrino states» although for our purposes this is almost insignificant. The flux of neutrinos is proportional to u⃗ 2\vec u^{\,2}. Notice that the frequency ω\omega and wavevector k⃗\vec k of the wave are related to the energy and momentum of neutrinos by the common quantum formulae: E=ℏωE=\hbar\omega and p⃗=ℏk⃗\vec p=\hbar\vec k, where ℏ\hbar is Planck constant.

The difference of frequencies is due to difference in masses: for the same momentum E1,2=m1,22c4+c2p⃗ 2=ℏω1,2E_{1,2}=\sqrt{m_{1,2}^2c^4+c^2\vec p^{\,2}}=\hbar\omega_{1,2}. Obviously, an orthogonal «polarization» u⃗1,2\vec u_{1,2} corresponds to the neutrino state of certain mass m1,2m_{1,2}. Notice, that states of definite flavor (νe\nu_e and νμ\nu_\mu) correspond to another pair of orthogonal «polarizations» u⃗e,μ\vec u_{e,\mu} which do not coincide with u⃗1,2\vec u_{1,2}.

The polarizations u⃗1,2\vec u_{1,2} corresponding to certain masses and polarizations u⃗e,μ\vec u_{e,\mu} corresponding to certain flavors are related as:

{u⃗1=u⃗ecos⁡ϑ−u⃗μsin⁡ϑ,u⃗2=u⃗esin⁡ϑ+u⃗μcos⁡ϑ.\begin{cases}\vec u_1=\vec u_e\cos\vartheta-\vec u_\mu\sin\vartheta,\\\vec u_2=\vec u_e\sin\vartheta+\vec u_\mu\cos\vartheta.\end{cases}

Angle ϑ\vartheta is called the «mixing angle» of νe\nu_e and νμ\nu_\mu. In this case νe\nu_e and νμ\nu_\mu indeed do not have «certain» masses and do not have a certain energy for a given momentum. For instance, a measurement of the energy of electron neutrino would «on average» yield the value

⟨Ee⟩=E1cos⁡2ϑ+E2sin⁡2ϑ=E−ΔE2cos⁡2ϑ,\langle E_e\rangle=E_1\cos^2\vartheta+E_2\sin^2\vartheta=E-\frac{\Delta E}{2}\cos2\vartheta,

where E≡(E1+E2)/2≈c∣p⃗∣E\equiv(E_1+E_2)/2\approx c|\vec p| is the mean neutrino energy and ΔE≡E2−E1\Delta E\equiv E_2-E_1. Such an outcome could be interpreted as being due to interaction of the states νe\nu_e and νμ\nu_\mu, where the interaction energy is Veμ=ΔEsin⁡ϑcos⁡ϑV_{e\mu}=\Delta E\sin\vartheta\cos\vartheta.

The quantities introduced above can be expressed in terms of energy EE and parameters m≡(m1+m2)/2m\equiv(m_1+m_2)/2, Δm≡m2−m1\Delta m\equiv m_2-m_1, and ϑ\vartheta. It has been already mentioned that accurate values of these parameters are not known yet but to solve the problem it would suffice to adopt the following approximate values: mc2=4,0⋅10−3 eVmc^2=4{,}0\cdot10^{-3}\ \mathrm{eV}, Δmc2=3,0⋅10−3 eV\Delta mc^2=3{,}0\cdot10^{-3}\ \mathrm{eV}, and ϑ=10∘\vartheta=10^\circ.

1) Evaluate «mean» masses of electron and muon neutrinos for the given values of the parameters. The answer can be given either in kg or eV/c².

Now consider neutrinos radiated from some small region and propagating along xx-axis. Let the energy of a neutrino created in this region be E≈2 MeVE\approx2\ \mathrm{MeV}, all created neutrinos are electron neutrinos and have the same certain momentum (this means that neutrinos are created with different masses and, therefore, energies). Clearly, the neutrino wave propagating along xx-axis is a mixture of neutrino waves corresponding to neutrinos of different masses (hence, a mixture of waves with certain frequencies at a given wavelength). The phase shift of the waves varies with distance xx. Since the phase shift varies the contributions to the resulting wave due to electron and muon component would vary as well. Therefore, at any particular position xx one would detect not only electron neutrinos but muon neutrinos as well. The intensities of the corresponding neutrino fluxes vary periodically in space. This phenomenon is called neutrino oscillations. [6 т.]

2) Determine the oscillation length, i.e. the period of spatial variation of the time averaged flux of muon neutrinos. The answer should be given as the formula and the numerical value (in meters). [5 т.]

Part II: neutrinos and the Sun.

Oscillations described in Part I occur in vacuum. At first glance, it would be reasonable to assume that matter does not alter the picture significantly since neutrinos very weakly interact with any matter which density is much less than the density of atomic nucleus. There is a powerful neutrino source close to the Earth. It is the Sun. Nuclear reactions proceed in the central region of the Sun suppling it with energy and creating neutrinos and antineutrinos, mostly, electron ones. However, the observed flux of electron neutrinos turned out to be only a half of the flux predicted from the Solar luminosity. Is it possible to explain this «deficit» by partial conversion of electron neutrinos to neutrinos of other flavors on their way from the Sun to the Earth (vacuum oscillations)?

3) Try to give a justified answer by using the data and the results from Part I of the problem. Do necessary calculations to support your judgement. In particular, it is reasonable to assume that energies of neutrinos created in nuclear reactions in the Sun are not very different from 2 MeV. Take into account the fact that a neutrino detector accumulates data for a long period of time, up to 2-3 months. The answer should be given as «+» (yes) or «–» (no).

A detailed analysis must take into account that the neutrinos travel a part of their path inside the solar substance. It turns out, absorption of the neutrinos by the substance does not change much the estimate for the flux of electron neutrinos but there is some additional circumstance which is quite essential. The solar substance contains a lot of electrons (see the problem data) and electron neutrinos interact with them much stronger than muon neutrinos do. Due to this fact the «mean» energy of electron neutrinos increases by δE\delta E, the quantity which is proportional to the electron density: δE≈1,27⋅10−12ne1031 m−3 eV\delta E\approx1{,}27\cdot10^{-12}\frac{n_e}{10^{31}\ \mathrm{m^{-3}}}\ \mathrm{eV}. At the same time the «mean» energy of muon neutrinos and the energy of interaction between the states νe\nu_e and νμ\nu_\mu remain practically the same. [2 т.]

4) Evaluate «new» value of mixing angle ϑ~\widetilde\vartheta (by taking into account the solar electrons). The answer should be the equation. [5 т.]

5) By how many percent can the solar electrons change the expected «deficit» of the electron neutrino flux? Evaluate in percent (%) the maximum increment of the flux of muon neutrinos due to oscillations (compared to the flux in the absence of matter). [4 т.]

6) Plot an approximate dependence (i.e. show only the main features) of the mass difference of νμ\nu_\mu and νe\nu_e as a function of the distance rr traveled inside the Sun from the center outwards.

Complete native blank response plot for neutrino mass difference, axes r/RC and m_mu−m_e, 0/0.5/1 marks and all dashed grid lines.

[3 т.]

Part III: neutrino and Supernova explosion.

After an «ordinary» star has exhausted its nuclear fuel the star cools down and its internal pressure cannot withstand gravitational compression anymore. As a result, the star is contracting until its substance undergoes transition to a new phase in which all electrons are «shared», all nuclei «float» in the electron «gas», and only the pressure of this gas halts further collapse.

The star can exist in this state for a long time; however, if the mass of its dense core gradually increases and exceeds Mcr≈1,5MCM_{\mathrm{cr}}\approx1{,}5M_C the core becomes unstable and collapses. At the onset of collapse such a core usually has a radius about 10000 km with approximately equal numbers of protons and neutrons. Soon after the contraction starts the rate of electron-nuclear collisions becomes high, which results in neutronization of the star substance due to reaction of «inverse β\beta-decay» (p+e→n+νep+e\to n+\nu_e). Electron disappearance reduces the pressure of electron gas accelerating the neutronization even more. The whole process is essentially the tremendous explosion leaving in the aftermath a neutron star and an «outer envelope» flying outwards. Astronomers call such an explosion «Supernova explosion» or simply «Supernova». A neutron star is indeed composed mostly of tightly packed neutrons, so its density is approximately equal to the density of atomic nuclei.

7) Estimate an order of magnitude of the energy released due to compression of the stellar core from the initial radius to the neutron star. Calculate the numerical answer in Joules.

The released energy converts to kinetic energy of the star remnants (the flying outer layers and rotation of the neutron star) and to the energy of electromagnetic radiation and neutrinos. Supernova explosion is one of the most powerful source of neutrinos (sometimes it is called «neutrino bombs»), calculations show that more than half of the released energy converts to the energy of radiated neutrinos. Neutrinos are radiated both at the neutronization stage and after formation of the neutron star which is initially extremely hot and subsequently cools down mostly by radiating neutrinos. The neutronization and cooling take just several seconds. Notice that only electron neutrinos are created during neutronization, and the neutrino-antineutrino pairs of various flavors are created during the cooling. [4 т.]

8) Estimate the number of neutrinos created by a Supernova explosion assuming that the mass of the initial stellar core is approximately 1,5MC1{,}5M_C (the stellar substance does not «go away» with outer layers), the energy of radiated neutrinos is 80% of the released energy, and the mean energy of radiated neutrinos and antineutrinos is approximately 10 MeV. You could assume that neutron mass and radius are approximately the same as those of proton. Calculate the numerical values. [4 т.]

9) Supernova SN1987А exploded at the distance of R≈50 kpcR\approx50\ \mathrm{kpc} from the Earth (in the Large Magellanic Cloud). What is the total number of neutrinos and antineutrinos passed through an Earth based detector of the cross-sectional area S=100 m2S=100\ \mathrm{m^2}? Estimate the expected number of detected neutrinos and antineutrinos assuming that the detector on average registers α=3⋅10−14%\alpha=3\cdot10^{-14}\% of neutrinos of any flavor in the corresponding energy range. Calculate the numerical values.

It is important that neutrino radiation is asymmetric with respect to the star magnetic axis due to «peculiar» neutrino behavior under mirror reflection: the power dIdI radiated in the infinitesimal solid angle dΩ=sin⁡θ dθ dϕd\Omega=\sin\theta\,d\theta\,d\phi is dI/dΩ=I4π[1+κ⋅cos⁡θ]dI/d\Omega=\frac I{4\pi}[1+\kappa\cdot\cos\theta], where κ≈10−2\kappa\approx10^{-2}, θ\theta is the angle of neutrino emission to the axis, and ϕ\phi is the angle of rotation around the axis. [2 т.]

10) Estimate the speed gained by the star due to neutronization and cooling. Calculate the numerical answer (in km/s). [5 т.]

Решение


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