3-1 RDCH 702: Lecture 3, Nuclear Reactions Readings: Modern Nuclear Chemistry, Chapter 10; Nuclear and Radiochemistry, Chapter 4 Notation Energetics of.

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Presentation transcript:

3-1 RDCH 702: Lecture 3, Nuclear Reactions Readings: Modern Nuclear Chemistry, Chapter 10; Nuclear and Radiochemistry, Chapter 4 Notation Energetics of Nuclear Reactions Reaction Types and Mechanisms §Barriers §Scattering Nuclear Reaction Cross Sections Reaction Observables Scattering Direct Reactions Compound Nuclear Reactions Photonuclear Reactions Nucleosynthesis

3-2 Nuclear Reactions Nucleus reactions with a range of particles §Nucleus, subatomic particle, or photon to produce other nuclei §Short time frame (picosecond) §Energetics involved in reaction First nuclear reaction from Rutherford §What reaction was this? Number of terms conserved during nuclear reactions §Basis for understanding and evaluating reactions àNumber of nucleons *except in reactions involving creation or annihilation of antinucleons àCharge àEnergy/Mass àMomentum àAngular momentum àParity Q is the energy of the reaction §positive Q corresponds to energy release §negative Q to energy absorption Q terms given per nucleus transformed Shorthand:

3-3 Energetics Energetically many orders of magnitude greater than chemical reactions 14 N( ,p) 17 O; Q= MeV §Convert energy to per molar basis à1 eV = 1.60E-19 J à=-7.18E23 MeV/mole= -7.18E29 eV/mole à=-1.15E11 J/mole Reactions so large that mass change is observable Q value can be experimentally measured to provide a route to determine particle mass of reactants §Mass and energy balance àKnow Q value, determine unknown mass

3-4 Energetics Reaction Q values §Not necessarily equal to kinetic energy of bombarding particles for the reaction to occur àNeed more energy than Q value for reaction to occur *Reaction products will have kinetic energy that needs to come from reaction Conservation of momentum §Some particles’ kinetic energy must be retained by products as kinetic energy Amount retained as kinetic energy of products §Based on projectile mass §Retained kinetic energy becomes smaller with increasing target mass àEquation for kinetic energy (T): What does this mean about reaction §Heavier target or heavier projectile? à 248 Cm + 18 O  266 Rf 248 Cm Projectile 18 O Projectile

3-5 Energetics: Reaction Barrier Need to consider laboratory and center of mass frame Laboratory frame §conservation of momentum considers angle of particles Q value can be found if T x and  are measured and particles known §T p from experiment Center of mass §Total particle angular momentum is zero Kinetic energy carried by projectile (T lab ) is not fully available for reaction §T lab - T cm = T 0 § T 0 is energy to be dissipated in reaction For reaction to occur Q + T 0 must be achieved §Basis for threshold reaction §Q + T 0 > 0

3-6 Reaction Barrier Threshold energy (minimum energy for reaction) Fraction of bombarding particle’s kinetic energy retained as kinetic energy of products becomes smaller with increasing mass of target §Heavier target or heavier projectile? § 248 Cm + 18 O  266 Rf Solve of laboratory T A for mass

3-7 Reaction Barrier: Threshold Energy Consider the 14 N( ,p) 17 O reaction §Find threshold energy àQ from mass excess *Q= – – (-0.809) = MeV Reaction barrier also induced by Coulomb interaction §Need to have enough energy to react and overcome Coulomb barrier àFrom charge repulse as particle approach each other *R is radius *r o =1.1 to 1.6 fm Equation can vary due to r o V c can be above threshold energy Center of mass, need to bring to laboratory frame §Consider kinetic energy carried by projectile §3.36x ((14+4)/14) = 4.32 MeV alpha needed for reaction

3-8 Equations for production reactions: Cross Sections Probability of a nuclear process is generally expressed in terms of a cross section  §dimensions of an area Originates from probability for reaction between nucleus and impinging particle is proportional to the cross-sectional target area presented by the nucleus §Doesn’t hold for charged particles that have to overcome Coulomb barriers or for slow neutrons Total cross section for collision with fast particle is never greater than twice the geometrical cross- sectional area of the nucleus  cross section  is close to 1 barn for this case cm 2 =1 barn

3-9 Cross sections Accelerator: beam of particles striking a thin target with minimum beam attenuation When a sample is embedded in a uniform flux of particles incident on it from all direction, such as in a nuclear reactor, the cross section is defined: §R i = # of processes of type under consideration occurring in the target per unit time §I= # of incident particles per unit time §n= # of nuclei/cm 3 §x=target thickness (cm) §  =flux of particles/cm 2 /sec §N=number of nuclei contained in sample

3-10 Production of radionuclides   =cross section   =neutron flux §t=time of irradiation   1-e -( t) ) *maximum level (saturation factor) Activity of radioactive product at end bombardment is divided by saturation factor, formation rate is obtained  R=A/  1-e -( t) ) half life%

3-11 Nuclei production: Short irradiation compared to half-life Find amount of 59 Fe (t 1/2 =44.5 d, = 1.803E-7 s -1 ) from irradiation of 1 g of Fe in a neutron flux of 1E13 n/cm 2 /s for 1 hour  58 Fe(n,  ) 59 Fe: 58 Fe+ n   + 59 Fe  1.3E-24 cm 2 §N o = 1g/ g/mol *6.02E23 atom/mol* § N o =3.04E19 atom R= 1E13 n/cm 2 /s *1.3E-24 cm 2 * 3.04E21 atom R=3.952E8 atoms/sec 1.423E12 atoms 59 Fe in 1 hour

3-12 Nuclei production: Long irradiation compared to half-life Find amount of 56 Mn (t 1/2 =2.578 hr, = 7.469E-5 s -1 ) from irradiation of 1 g of Mn in a neutron flux of 1E13 n/cm 2 /s for 1 hour  55 Mn(n,  ) 56 Mn: 55 Mn+ n   + 56 Mn  13.3E-24 cm 2 §N o = 1g/ g/mol *6.02E23 atom/mol § N o =1.096E22 atom R= 1E13 n/cm 2 /s *13.3E-24 cm 2 * 1.096E22 atom R=1.457E12 atoms/sec 5.247E15 atoms 56 Mn in 1 hour (does not account for decay)

3-13 Formation rate from activity R=A/  1-e -( t) ) 4.603E15 atoms 56 Mn (t 1/2 =2.578 hr, = 7.469E- 5 s -1 ) from 1 hour irradiation A= N= 4.603E15* 7.469E-5 =3.436E11 Bq R=A/  1-e -( t) ) R= 3.436E11/(1-exp( E-5 *3600)) R=1.457E12 atom/sec

3-14 Cross Section Values and Limits Reaction cross section of  R 2 is approximated at high energies §Wave nature of incident particle causes upper limit of reaction cross section to include de Broglie wavelength àSo cross section can be larger than area due to incoming particle wavelength àExpressed as an increase in R, quantum in nature Collision between neutron and target nucleus characterized by distance of closest approach §B is impact parameter

3-15 Cross sections Angular momentum of system is normal to the relative momentum p b any value between 0 and R l =0,1,2,…b angular momentum §lħ Sum all l from 0 to l max Cross section based on summation of l cross sections For this reason nuclear reaction cross sections can be several orders of magnitude larger than the nuclear geometrical cross section §Manifest by slow-neutron reactions

3-16 Cross section Quantum-mechanical treatment T is the transmission coefficient for reaction of a neutron with angular momentum  Represents fraction of incident particles with angular momentum that penetrate within range of nuclear forces àProvides summing term to increase cross section àReason why cross section can be larger than physical size of nucleus  l is partial cross section of given angular momentum l General trends for neutron and charged particles §Charged particle cross section minimal at low energy §Neutron capture cross section maximum at low energy

3-17 Measuring Cross Section: Excitation Functions Variation of reaction cross section with incident energy Shape can be determined by exposing several target foils in same beam with energy- degrading §Simultaneous measurement of multiple particle energies Provide information about probabilities for emission of various kinds and combination of particles in nuclear reactions §formation of given product implies what particles were ejected from target nuclide Range of cross sections can be evaluated §Detection limit of product can influence cross section limit measurement

3-18 Barriers for Charged Particles Coulomb repulsion between charged bombarding particles and nucleus §Repulsion increases with decreasing distance of separation until charged particle comes within range of nuclear forces §Probability of tunneling through barrier drops rapidly as energy of particle decreases §Coulomb barriers affect charged particles both entering and leaving the nucleus àCharged particles emitted from nuclei experience Coulomb repulsion during emission àgreater than 1 MeV àseen with position emission Related to change in cross section with energy for charged particle reactions §Maximum cross section dependent upon energy