1 / 28

Neutron Resonance States in Overdense Crystals

Neutron Resonance States in Overdense Crystals. N.Takibayev Institute of Experimental and Theoretical Physics, Kazakh National University, Almaty , Kazakhstan nur.takib@gmail.com.

warner
Download Presentation

Neutron Resonance States in Overdense Crystals

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Neutron Resonance States in Overdense Crystals N.Takibayev Institute of Experimental and Theoretical Physics, Kazakh National University, Almaty, Kazakhstan nur.takib@gmail.com

  2. New type resonances of light particle in systems of heavy centers have been obtained in the framework of model problems that admit exact solutions. See: Takibayev N.Zh. “Class of Model Problems in Three-Body Quantum Mechanics That Admit Exact Solutions”// Physics of Atomic Nuclei, V 71, No 3, p 460-468, 2008 The resonance energies and widths are shown depend on distances between heavy centers. Takibayev N.Zh., Exact Analytical Solutions in Three-Body Problems and Model of Neutrino Generator, EPJ Web of Conferences, V 3, 05028, p 1– 8, (2010); arXiv: 1002.2257v1 [nucl-th]. Takibayev N "Neutron resonanses..."

  3. In the case of neutron the new resonance states appear in subsystem of heavy fixed nuclei when these distances are many times more than the radius of nuclear forces and many times less than the atomic size. Takibayev N.Zh., Neutron Resonances in Systems of Few Nuclei and Their Possible Role in Radiation of Overdense Stars, Few-Body Systems,Springer-Verlag, Springer ed., DOI: 10.1007/s00601-010-0207-4, 2011 Therefore, new neutron resonance states can take place in overdense crystals, for instance, inside of overdense star crusts or cores. Parameters of these resonances in two nuclei subsystems of Mn, Ti, Fe, Ni and some others and their radiation spectra have been calculated. Takibayev N "Neutron resonanses..."

  4. Problems whose solutions are known in an analytic form are of paramount importance since they permit performing a transparent investigation into phenomena. Model problems can result in unusual and unexpected solutions. A generalization of such model solutions can provide an efficient tool for studying more complicated systems, this being of importance for a number of practical applications. Model problems are also of interest as tests of various numerical methods. Solutions to these problems may be of interest for a number of problems in atomic and molecular physics, as well as some problems in crystal physics, nuclear physics, and nuclear astrophysics. Takibayev N "Neutron resonanses..."

  5. Class of Model Problems in Three-Body Quantum Mechanics That Admit Exact Solutions • Here we consider a very simple model of three particle system. • This model is based on two simplifying approximations: • two-particle interactions are taken in the form of separable potentials; • in three-particle system Born-Oppenheimer approximation is used. • The first approximation gives the exact solution of the two- particle problem at once in an analytical form. • The second one leads to a simplification of the three-particle problem in the assumption that one particle is light, while the others are heavy. Takibayev N "Neutron resonanses..."

  6. The first approximation assumes that two-body interactions have separable or “compound” form. where the enhancement factor η = η(E) depends on the initial energy only: The amplitude of Breit-Wigner form corresponds to such definition where Index “2” marks parameters of two-body system Takibayev N "Neutron resonanses..."

  7. The second (Born-Oppenheimer) approximation (the limit of ) results in simplification of three-body equations. And together two approximations leads to exact solutions of three-body problem. Then we introduce the Fourier transform of three-body equations (see in Physics of Atomic Nuclear, V 71, pp 460-468, 2008) and obtain: where - initial momentum of the light particle, and l,k = 2,3. Takibayev N "Neutron resonanses..."

  8. The solutions of problem of light-particle scattering on two fixed centers can be represented in the analytical form. We can write out the two modes of solution: where Elements of diagonal matrix are where i,j = 2,3 – numbers of heavy centers, r, r’ - radius-vectors of the initial and final fixed scattering centers, respectively. Takibayev N "Neutron resonanses..."

  9. Now we consider the problem of neutron scattering on two fixed centers subsystem if the two-body scattering amplitudes have the Breit-Wigner resonant form: The energy and width of resonance are determined with real and imaginary parts of resonance wave number: Here, index 2 marks two-body parameters (below index 3 will mark three-body parameters). The BW representation can be transformed to separable form if determine a form-factor as Takibayev N "Neutron resonanses..."

  10. Then we obtain So, three-body exact solutions can be obtained in case of Breit-Wigner pair t-matrices, too. Let we have an isolated pair resonance acting in S-wave. Then we can write the elements of matrix J as Zeros of D are determined by equation And we mark values of when Takibayev N "Neutron resonanses..."

  11. There are two sets of three-body resonances: Some of them are situated at energy scale above the energy of two-body resonance, and others - under this energy. Some of three-body resonances will have more narrowed width, others – more widened in comparison with the width of two-body resonance Note, there are no principal difficulties in including more complicated forms of two-body separable potentials and other partial components into the model. Takibayev N "Neutron resonanses..."

  12. In common case of neutron-nucleus resonance scattering we have to take into account not only elastic scattering: but inelastic channels too. First of all we take into account the reactions of gamma radiations via neutron resonance capture : where is exited nucleus of mass number bigger than . Then resonance part of two-body t-matrix can be represented in Breit-Wigner’s form, as: Takibayev N "Exact Analytic Solutions..."

  13. It is remarkable that our consideration of new three-body quantum states remains without modifications. Really, the neutron capture by nucleus (as a two-body reaction) leads to disappearance of neutron as the main particle in three-body rescattering. So, the process of three-body rescattering, which gives new quantum states, will stop after the act of neutron capture. We guess that a probability of neutron appearance via inverse reaction will be very small: Therefore, the function ( - the enhancement factor of three-body amplitude) is the result of neutron elastic rescattering on subsystem of heavy centers. Takibayev N "Exact Analytic Solutions..."

  14. However, three-body inelastic reactions will be connected with elastic one and all of them will have resonance behavior at the same resonance points depending on values of It means that new type of gamma radiation will appear under the same conditions as three-body neutron resonances where function We can write a coupled part of three-body inelastic amplitude in form where as above Takibayev N "Exact Analytic Solutions..."

  15. It is important to note that matrix is the effective potential created by the light particle (neutron) rescattering between two-heavy centers (ions in nodes of dense crystal). This effective potential with resonance behavior becomes very strong at resonance points and can be many times more than ordinary direct two-body interaction, for example, the Coulomb repulsive forces between ions. We consider results of calculations for the neutron resonances inside of solid structure. Nucleus will be assumed fixed in the nodes of the crystal lattice. Our calculations are based on the well-known data of neutron-nucleus resonances. The lowest neutron-nucleus resonances, which are well isolated from each other, have been taken into account. Takibayev N "Neutron resonanses..."

  16. The important quantity of the three-body problem is because K is the universal factor in amplitudes Moreover this factor determines the ratio of three-body and two-body amplitudes under the same conditions. Takibayev N "Neutron resonanses..."

  17. The n+ Mn55 + Mn55 three-body system • The lowest resonances in two-body subsystems of n+Mn55 • with J=3 ; l = 0 : • bound states with energy: Eb1= - 5.1 keV in S-wave, • the first resonance: ER = 1,098 keV; G = 18 eV ; Gn = 18 eV; • the second resonance : ER = 2,37 keV, G =Gn = 460 eV ; • 2) with J=2 ; l = 0 • bound states with energy: Eb2=- 2.4 keV in S-wave, • the first resonance: ER = 0,336 keV and Γ =(18,3+0.435 ) eVΓn = 18.3 eV ; Takibayev N "Neutron resonanses..."

  18. Three-body resonances in the case of J=3, l=0 Im (K) Re (K) k0 = kR*(1+y); the parameter y give a deviation y = k0/kR-1 Here the distance between ions of Mn55: d=r/2, r - in fm Takibayev N "Neutron resonanses..."

  19. Three-body resonances in the case of J=2, l=0 Im (K) Re (K) k0 = kR*(1+y); the parameter y give a deviation y = k0/kR-1 Here the distance between ions of Mn55: d=r/2, r - in fm Takibayev N "Neutron resonanses..."

  20. The n+ Fe56 + Fe56 three-body system; • The lowest resonances in two-body subsystems n+Fe56: • bound states with energy: Eb= - 6.52 keV in S-wave, • the first resonance : ER = 1,147 keV and G = 0.74 eV ; Gn = 0.056 eV ; • 3) the second resonance: ER = 12,45 keV G = 0.0023 eV= Gn Re (K) Im (K) Takibayev N "Neutron resonanses..."

  21. The n+ Fe57 + Fe57 three-body system; • The lowest resonances in two-body subsystems n+Fe57: • bound states with energy: Eb= - 0.44 keV in S-wave, J=1 • the first resonance : ER = 1,63 keV and G = 0.11 eV =Gn ; • 3) the second resonance: ER = 3,95 keV G = 108 eV= Gn Im (K) Re (K) Takibayev N "Neutron resonanses..."

  22. The n+ Ni61 + Ni61 three-body system • The lowest resonances in two-body subsystems n+Ni61: • bound states with energy: Eb= - 0.0095 keV in S-wave, J=2 • the first resonance : ER = 7,545 keV and G = 227,3 eV • Gn = 225 eV ; Im (K) Re (K) Takibayev N "Neutron resonanses..."

  23. The three-body system: n+ Ni62 + Ni62 • The lowest resonances in two-body subsystems n+Ni62: • - bound states with energy: Eb= - 0.077 keV in S-wave, J=1/2 • the lowest resonance : ER = 4,54 keV ; G = 1880 eV =Gn Im (K) Re (K) Takibayev N "Neutron resonanses..."

  24. The three-body system: n+ Ni62 + Ni62 A wider range of r : (10 – 500) fm. Re (K) Im (K) Takibayev N "Neutron resonanses..."

  25. The resonant nature of the effective interaction may lead to the following interesting phenomena. If the distance between the nuclei in solid structure is close to the , the resonance will be evolving rapidly. The structure will collect plenty of structural resonance neutrons. Their multiple rescattering on nuclei of structure will be accompanied by the radiation capture of neutrons. There will be a resonant gamma radiation. Takibayev N "Neutron resonanses..."

  26. Effect resonance scattering of light particle on two heavy centers when distance between centers can be changed d =2r In the case of a single crystal under high pressure, the collective effects create a series of resonant states for neutrons in the crystal.

  27. As a result, the resonant structure will release energy. Released energy and radiation will spread inside the neutron star. But by raising the temperature the structure volume will increase. Therefore, the structure will leave the resonance property of energy generation. Then the structure begins to cool down and returns to former state with the parameters close to the resonance. Takibayev N "Neutron resonanses..."

  28. The resonance cycle can be repeated over and over again. It will be a kind of "breathing" of star solid structures. Acknowledgments. I thank Prof. Kiyoshi Kato and the group of “Nuclear Reaction Asia Database“ for useful discussions, the Hokkaido University for their hospitality and support, and Prof. M. W. Snow for his valuable advices. Thank you for your attention! Takibayev N "Neutron resonanses..."

More Related