5 What holds nucleus together? The answer was proposed by Hideki Yukawa in 1935, he called it a STRONG NUCLEAR FORCE.It is exerted by the p+ and n0 on each otherSNF overwhelms the electrostatic charge (++)
6 SNFThe SNF acts over very short distance, so larger nuclei the force does not reach far enoughIf the SNF is not enough, the electrostatic forces will dominate and the nucleus will break apart.Instability occurs when nucleus is too big
7 Nuclear symbolsChapter 19 requires that you understand nuclear symbols and how to manipulate them.AXZ
8 Nuclear vs Chemical Reactions In a chemical reaction:Atoms are rearranged to form new substancesIn nuclear reactions:We are creating new elements!ALCHEMY!
9 Radioactive DecayRadioactive – something is radioactive if the nucleus spontaneously decomposesWhen it does this a different nucleus is formedExtra particles are usually formed alsoExample:The symbol represents a beta (b) particle
10 b particle productionThe mass of a beta particle is 0, and the atomic number is –1:So, beta particles change neutrons to protons.
11 Where did the e- come from? A decaying neutron!!!
12 Nuclear equations & Laws Notice that in the equation, atomic mass (A) and atomic # (Z) are the same on both sides of the arrow.Law of conservation of Mass!
13 Types of Radioactive Decay Alpha (a) particle: An alpha particle is a Helium Nucleus.The nuclear symbol is:
14 Gamma Rays (g) A gamma ray is a high energy photon of light. Released along with other types of radiation
15 PositronsA particle with the same mass as an e- but a positive charge:Positrons are anitmatter!Example:
16 Electron capture A nucleus CAPTURES an inner electron Gamma rays are always produced.Explanation:NOTE that in electron capture the beta particle is always on the LEFT of the arrow!!
17 Decay SeriesAn unstable nucleus undergoes a series of changes until it becomes a stable nucleus
18 Band of StabilityPredicts whether or not an atom’s nucleus will be stable.For atoms less than 20 p+, n0:p+ are 1:1n0/p+ ratio greater than 1.5/1 will be unstable
19 Binding Energy & Mass Defect Binding Energy – energy that holds nucleus togetherMass defect – the ‘missing mass’ when the mass of nucleons are added together.Example: Iron – 56
20 E = mc2 Einstein’s idea E = energy m = mass in kilograms c = speed of light 3x108 m/s
28 Nuclear Fusion Produces more energy than fission! Takes very high temperatures to get protons close enough to “stick” to each otherWhy is “cold fusion” a hollywood fad?
29 Effects of Radiation Different particles penetrate in different ways energymassHow easily they make ionsChemical propertiesThese things make radiation more or less harmful
30 Detecting RadiationHigh energy particles from radioactive decay make ions when they travel through matter.The fast particles “knock” electrons off the atoms they hit.A geiger counter can detect these ions through the flow of electricity
32 Carbon Dating (Radioactive Dating) Based on the radioactivity of carbon-14, which decays through b-particle production.Carbon-14 is continuously made in the atmosphere when neutrons from space hit the nitrogen in the air.
33 More on carbon dating:Living things always have the same amount of C-14 because they take it in through the air.As soon as a living thing dies it stops taking in carbon from the atmosphere. The C-14 decays.The ½ life of C-14 is 5730 years.If a piece of wood has ½ the C as a living tree, it is 5730 years old.What are some of the problems with this method?
34 Making new elementsScientists make new elements by bombarding existing nuclei to create elements with larger and larger atomic numbers.
35 Changing one element into another Radioactive decay is when a nucleus decomposes and turns in to another nucleusBombarding nuclei with particles can form new nuclei also.