ACNS 2008 Tutorial Section SANS and Reflectometry for Soft

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ACNS 2008 Tutorial Section SANS and Reflectometry for Soft Condensed Matter Research The Basic Theory for Small Angle Neutron Scattering Wei-Ren Chen Neutron Scattering Sciences Division Spallation Neutron Source Oak Ridge National Laboratory May 11th 2008 Outline  Two Aspects of Collision: Kinematics vs. Dynamics  Cross Section Calculation I: Method of Phase Shift  Cross Section Calculation II: Fermi Approximation  Expression of Scattering Cross Section s(q)  Coherent and Incoherent Scattering  Contrast variation  References Kinematics Aspect of Collision 12 variables: v1, v2, v1’ & v2’ v1’ v2 particle 2 (target) particle 1 (projectile) v1 Conservation laws • energy (1) • mass(1) • momentum (3) • v1 and v2 are known (6) v2’ 1+1+3+6 = 11 Kinematics Aspect of Collision Possible existence of Neutron James Chadwick Nature, 129, 312, 1932 closest approach effective particle 1 1    m1 m2 1  Is this reaction possible?  Does it violate any conservation law? Independent of the specific forces between the particles origin What is the possibility that the projectile will scatter off the target at that specific angle? Interaction: hidden in Cross Section scattering ≡ (initial constellation = final one), elastic scattering ≡ conservation of kinetic energy A+ B→A+ B Dynamics Aspect of Collision: Concept of Cross Section d  d dq area A q polar axis Beam size A (L2) Intensity of beam I (T-1) Thin sample thickness Δx (L) Number density of sample N (L-3) no. of reaction occurring per second Q (T-1) Reaction probability ≡ Intensity I density N x Q NAx  I A azimuthal axis Q  NAx    s I  A  s : a proportionality constant of reaction probability with dimension of L2 To calculate s one must be to be able to calculate reaction probability Scattering Experiment * J in  vin in  v e ikr sc  f (q ) r J sc  v sc  v * sc f (q ) 2 R2 * dN  (vsc sc )R 2 d ds dN / d 2 s (q )    f (q ) d J in angular differential cross section in  e i k r  e ikz ds s   d d Given the interaction potential V(r), how can one calculate σ(θ)? Phase Shift Analysis Schrödinger equation: Where is f(θ) in Schrödinger equation ?  2 2     V (r )   E   2  You put it in through boundary condition looking for far field solution (kr >> 1 , V(r) = 0) E > 0 LHS e ikz e ikr e ikr ikr cosq  f (q ) e  f (q ) r r RHS u 0 (r )  Al sinkr  (l / 2)  d l  d0 is introduced as one of the integration constants expanded by partial wave matching the coefficients of exp(ikr) and exp(-ikr) from RHS and LHS 1 s (q )  2 k  (2l  1)e l 0  id l sin d l Pl (cosq ) 2 and 4 s 2 k (2l  1)sin 2 d l  0  Reasoning of S-wave Scattering for Low Energy Scattering (kr0 << 1) v b z r0 Classically L  mbv  (1.67  1024 g ) (5  1013 cm) (106 cm / sec)  1030 erg  sec Quantum Mechanically l (l  1)  2  1027 erg  sec Only neutrons with l = 0 will be scattered Definition of Scattering Length a 1 s (q )  2 k  u0  (2l  1)e d i l 0  l sin d l Pl (cosq ) 2 and s 1 sin 2 d 0 when kr0  1 k2 4 sin 2 d 0 when kr0  1 k2 d0 → 0 as k → 0 a  lim  f (q )   k 0 d0 k d0 s (q )  a 2 sin(kr) sin(kr+d0) s  4a 2 Accurate Measurements of the Scattering Length http://physics.nist.gov/MajResFac/InterFer/text.html Physical Significance of Sign of Scattering Length u 0  A sin (kr  d 0 )  A sin (kr  ka)  Ak (r  a ) uo r0 a<0 0 a>0 r Example: Neutron-Proton Scattering Lecture 2 Basic Theory - Neutron Scattering for Biomolecular Science Roger Pynn, UCSB, 2004 Example: Neutron-Proton Scattering From the capture of a low-energy neutron by hydrogen V(r) r0=2F -EB 2.23 MeV r n + H1 → H2 + g (2.23 MeV) Solving the Schrödinger equation with this binding energy, (E < 0) V0 = -36 MeV and r0 = 2 F (F = 10-13 cm) -Vo 36 MeV Matching the wave functions and their flux for the exterior and interior regions, (E > 0) s = 2.3 barns Example: Neutron-Proton Scattering The “Barn Book” Brookhaven National Laboratory Report BNL-325, 1955 ~20 barns 2.3 barns Experimental Nuclear Reaction Data (EXFOR / CSISRS) National Nuclear Data Center http://www.nndc.bnl.gov/ Example: Neutron-Proton Scattering spin dependence interaction Eugene P. Wigner, Zeits. f. Physik 83 253 1933 triplet state (bound state) I = 1, parallel, EB = -2.23 MeV t singlet state (virtual state) I = 0, antiparallel, E* = 70 keV s (q )  1 3 2 1  sin d 0 T  sin 2 d 0S   k2  4 4  s = 20 barns Fermi Approximation Step 1 – Born Approximation Why we need Born Approximation? The many-body problem of thermal neutron scattering What is Born Approximation? Another way to solve the Schrödinger Equation eikr  (1) (r )  eikz  d 3r ' exp ( i k  r ')V (r ) exp (i k '  r ') 2r 2  Compare with eikr   e  f (q ) r ikz 2 f (q )   d 3r exp( i  r )V (r ) 4 2  Born approximation eliminates the need of solving Schrödinger equation Can Born Approximation be Applied to Neutron Scattering? V0 r02  2  1 If we use the potential parameters for n-p scattering V0 r02 2 1.6 10 24  36 10 6 1.6 10 12  4 10 26   3.7 54 10 No with real potential, too large for Born Approximation to be applicable Fermi Approximation Step 2 – Fermi Pseudopotential a   f (q ) kr 0 0 m  d 3rV (r ) ~ V0 r03 2 2  Fictitious potential V0* ~ 106 V0 r0* ~ 102 r0 Requirement Real potential kr0  1 kr0 ~ 10 4 kr0* ~ 102 V0 r02 2 V0 r03  constant  1 V0 r02 2 V0 r03  constant  3 .7 V0 r02 2 * *3 0 0  3  10 2  1 V r  V0 r03 With this fictitious potential, Born Approximation is valid Fermi Approximation Step 2 – Fermi Pseudopotential V(r) V(r) 0 a   f (q ) kr 0 m  d 3rV (r ) ~ V0 r03 2  2 2 2 V (r )  m *  b d (r  r ) N i 1 i i V0* ~ 10-6V0 r0* ~ 102r0 r0 * -V0 Why delta function? What is b ? r0 * actual neutron-nucleus interaction potential actural neotron-nucleus interaction potential -V0 Fermi pseudopotential Fermi 8 cm   10pseupotential r0 ~ 10 13 cm r0* ~ 10 11 cm Enrico Fermi, Ricerca Scientifica 7 13 1936 Neutron Scattering Data for Elements and Isotopes Neutron Diffraction George E. Bacon Chemical Binding Effect s ~ 2 1 1    mn mT 1 low energy (0.025 eV) 1 1   ~1  1 18( water)  ~1 1 high energy (~10 eV) 20  4  80 barns 1 1   2  1 1   0.5 1 20 barns Lecture 2 Basic Theory - Neutron Scattering for Biomolecular Science Roger Pynn, UCSB, 2004 A Typical Reactor-based SANS Diffractometer angular differential cross section ds s (q )  d Lecture 5 Small Angle Scattering - Neutron Scattering for Biomolecular Science Roger Pynn, UCSB, 2004 Expression of s(q): Coherent & Incoherent Contribution 2 2 V (r )  m *  b d (r  r ) N i 1 i i f (q )   2 d 3r exp( i  r )V (r ) 4 2  ds 2 s (q )   f (q )  d bi 2  b b i 1 j 1 i N N j exp  i k  ri  rj 2  ( )  b2 2  bcoh bi b j  bi b j  b b 2 (b 2 2  b 2 2 ) b 2 inc s (q )  N b 2  b ( ) b  exp( i k  r ) N i 1 i 2 2 2  Nbinc  Nbcoh S (k ) Example: Neutron-Proton Scattering s (q )  N b 2  b ( 2 ) b 2  exp( i k  r ) N i 1 i 2 2 2  Nbinc  Nbcoh S (k ) F= 10-13 cm s  I  1 1 or s  I  , magnatic quantum number : 2s  1 2 2 t b  (3b  b )  3  (5.4  2)  ( 23.7  2)  3.8F For H s  1 s  0 bcoh  b  3.8F  s coh  1.8 barns binc  b 2 (3b  4 2  b 4 2  )  649 F 4 2 (b 2  b 2 )  25 .5F  s inc  80 .2 barns b  (4b  2b )  4  (0.95)  2  (0.10)  6.7 F 6 4 3 1 s  For D s  2 2 s coh  5.6 barns b2  60.5F 2 s inc  2.0 barns Contrast Variation 10-12 F = 10-13 cm Neutron Diffraction George E. Bacon Basis of Contrast Variation For H For D For O b H  3.8F For H2O b D  6.7F b  5.8F For D2O b H 2O  1.8F t b D2O  19.2F b solvent can be adjusted to take on any value between these two extremes Scattering Length Density Calculator http://www.ncnr.nist.gov/resources/sldcalc.html F = 10-13 cm Lecture 1 Overview of Neutron Scattering & Applications to BMSE – Neutron Scattering for Biomolecular Science Roger Pynn, UCSB, 2004 References and Further Reading  Roger Pynn - An Introduction to Neutron Scattering (http://www.mrl.ucsb.edu/~pynn/) - Neutron Physics and Scattering (http://www.iub.edu/~neutron/)  Sidney Yip et al. - Molecular Hydrodynamics  Sow-Hsin Chen et al. - Interaction of Photons and Neutrons With Matter  Peter A. Egelstaff - An Introduction to the Liquid State  M. S. Nelkin et al. - Slow Neutron Scattering and Thermalization  Anthony Foderaro - The Element of Neutron Interaction Theory  Paul Roman - Advanced Quantum Theory  Jean-Pierre Hansen et al. - The Theory of Simple Liquids  Stephen W. Lovesey - Condensed Matter Physics: Dynamic Correlations  Peter Lindner and Thomas Zemb – Neutrons, X-rays and Light: Scattering Methods Applied to Soft Condensed Matter  Ferenc Mezei in Liquids, Crystallisaton et Transition Vitreuse, Les Houches 1989 Session LI  Léon Van Hove Physical Review 95 249 1954

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