Nuclear (Chang) Flashcards
Radioactivity
Unstable nuclei emitting particles/ electromagnetic radiation spontaneously
Radioactive elements
Atomic number greater than 83
Nuclear transmutation
Results from bombardment of nuclei by neutrons, protons, or other nuclei
Nuclear reactions
-radioactive decay and nuclear transmutation
(A) Chemical reactions
(B) Nuclear reactions
- (A) atoms are rearranged by the breaking and forming of chemical bonds
(B) Elements (or isotopes of the same elements) are converted from one to another
2.
(A) Only electrons in atomic orbitals are involved in the breaking and forming of bonds
(B) Protons, neutrons, electrons, and other elementary particles may be involved
- (A) Reactions are accompanied by absorption or release of relatively small amounts of energy
(B) Reactions are accompanied by absorption or release of tremendous amounts of energy - (A) Rates of reaction are influenced by temperature, pressure, concentration, and catalysts
(B) Rates of reaction normally are not affected by temperature, pressure, and catalysts
Nuclear stability
-nucleus: densest portion of atom (most mass, least volume)
-Coulomb’s law: like charges repel. But there are also SHORT RANGE ATTRACTIONS between prot-prot, prot-neut
-stability depends on the difference between coulombic repulsion and short range attraction
Neutron-to-proton ratio
-principal factor in nuclear stability
-low atomic number elements: n/p is close to 1
-⬆️ atomic number, n/p becomes greater than 1
-larger number of neutrons are needed to counteract strong repulsion among protons
Predicting nuclear stability
-Nuclei more stable if either proton/ neutron are:
2, 8, 20, 28, 50, 82, 126 (magic numbers)
-Nuclei with EVEN numbers of BOTH protons and neutrons are MORE STABLE than with ofd numbers
-Isotopes of elements with atomic number higher than 83 are radioactive: including Technetium (Z=43) and Promethium (Z=61)
Belt of stability
-# Neutrons vs # Protons
-stable nuclei
•above belt, nuclei with higher n/p ratio
-to lower ratio (move toward belt), undergo beta-particle emission (increase of proton, decrease neutron)
•below belt, nuclei with lower n/p ratio
-to increase ratio, undergo positron emission or electron capture
Nuclear binding energy
-quantitative measure of nuclear stability
-energy required to break up nucleus into its components protons and neutrons
-conversion of mass to energy that occurs during EXOTHERMIC NUCLEAR REACTION
∆E=∆mc^2
Energy/mass of product - energy/mass of reactant
Mass defect
-Difference between mass of an atom and the sum of the masses of its protons, neutrons and electrons
-masses of nuclei are always less than sum of the masses of nucleons (protons and neutrons)
-loss in mass is converted as energy released (negative energy)
Nuclear binding energy per nucleon
= nuclear binding energy (J)/ number of nucleons, protons+neutrons (nucleons)
-highest binding energies per nucleon: mass number 40-100 (esp. iron, cobalt, nickel region); highest attraction of protons and neutrins
Radioactive decay series
Sequence of nuclear reactions that ultimately result in the formation of stable isotope
•Parent: beginning radioactive isotope
•Daughter: profuct
Kinetics of radioactive decay
All radioactive decays obey FIRST ORDER KINETICS
-rate constants are unaffected by changes in environment (temp and pressure)
Radiocarbon dating (Uranium-238 Isotopes)
-estimating age of rocks in earth and extraterrestrial objects
-half-life of first step: U(238,92) ➡️ Th(234,90): 4.51x10^9 years (rate determining step; assume as half life for the overall process U(238,92) ➡️ Pb(206,82)
-estimate age of rocks from mass ratio of Pb(206,82) and U(238,92)
-if half mole of U(238,92) decayed, mass ratio=0.866
-higher ratio: rock exists longer than 4.51x10^-9 vice versa
Earth
4.5 x 10^9 years old
4.5 billion