nuclear chemistry
DESCRIPTION
Nuclear Chemistry. Ch.18. (18-1) Nuclear Stability. Nucleons : p + & n 0 Nuclide : any combo of p + & n 0 in a nucleus Isotope : same at.#, but different mass Te-122, Te-124, Te-128 Isobar : same mass, but different at.# Xe-124, Te-124, Sn-124. Binding Forces. - PowerPoint PPT PresentationTRANSCRIPT
Nuclear Chemistry
Ch.18
(18-1) Nuclear Stability
• Nucleons: p+ & n0
• Nuclide: any combo of p+ & n0 in a nucleus– Isotope: same at.#, but different mass• Te-122, Te-124, Te-128
– Isobar: same mass, but different at.#• Xe-124, Te-124, Sn-124
Binding Forces
• Strong nuclear force: attraction that holds nuclear particles together– Overcomes repulsive forces
Mass Defect
• Mass converted to E when a nucleus forms
Nuclear Binding E• E emitted when nucleons come together (E
needed to break a nucleus apart)
Band of Stability
• Area on a graph of n0 # v. p+ # in which all stable nuclei lie
Nuclei are more stable if they…
• Contain n0 ≥ p+
• Do not have too many or too few n0
• Have even #’s of nucleons• Have “magic #’s” of p+ or n0
– 2, 8, 20, 28, 50, 82, 126• Are not a neighboring isobar
(18-2) Types of Nuclear Change
• Spontaneous1. Radioactivity
– Artificial Transmutations2. Fission3. Fusion
• Nonspontaneous4. Transmutation
Radioactivity
• A nucleus decays & emits particles & electromagnetic waves
Converting n0 to p+
• Beta (β) decay: nuclei w/ too many n0 for the at.# become more stable by decaying & emitting radiation
• β particle: e- emitted from a nucleus when a n0 changes to a p+
• Ex:
Converting p+ to n0
• e- capture: nucleus has too few n0, so it absorbs an e-, which changes a p+ into a n0
• Gamma rays (γ): E produced by decaying nuclei
• Ex:
Converting p+ to n0 (cont.)
• Positron emission: nuclei emit postitrons (antiparticles of e-)
• Ex:
Annihilation of Matter
• Event when a particle collides w/ its anitparticle & both are changed into E
Losing Alpha Particles
• Alpha (α) decay: very large nuclei w/ too few n0 can decay by emitting α particles
• α particles: Helium-4 made when a n0 decays• Ex:
• Decay series: many heavy nuclei must decay several times before reaching a stable state
Balancing Nuclear Eq.’s
• Total mass #’s & nuclear charges must balance on both sides of the eq.
• Ex: Masses = 234, Charges = 90
• Ex: Masses = 238, Charges = 92
Nuclear Fission
• Rxn in which a large nucleus splits into 2 & produces a lot of E
• Chain rxn: nuclear rxn that sustains itself• Critical mass: smallest mass of radioactive
material needed to sustain a chain rxn
Nuclear Fusion
• 2 small nuclei combine to form 1 more stable nucleus & lots of E
• Reactants are plasmas (mixture of + nuclei & e-)
• Need very high T’s & P’s
Transmutation
• Creating new nuclei by bombarding a nucleus w/ α particles
• Produces an unstable cmpd that stabilizes by emitting a p+
(18-3) How Nuclear Chem is Used
• Radioactive dating: using radioactive isotopes to determine an object’s age
• Half-life: time required for half of a radioactive material to decay
Smoke Detectors
• Have an α emitter, which attract e- from the gas, changing them to ions which conduct electricity
• When smoke particles mix w/ the gas, they reduce current flow & the detector’s circuits are set off
Neutron Analysis
• Used to determine composition of objects– Meteorite composition– Forensic science (gun residue)
Radiation Exposure
• rem: biological effect of exposure to nuclear radiation– Limit of 5 rems/yr