Physics 12 Mr. Jean May 20th, 2014 The plan: Video clip of the day Question #1 –Visiting the Relatives Binding energy Energy Deflection Mass and energy.

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Presentation transcript:

Physics 12 Mr. Jean May 20th, 2014

The plan: Video clip of the day Question #1 –Visiting the Relatives Binding energy Energy Deflection Mass and energy

Chapter 20: Introduction The Nucleus & Radioactivity: –Nuclear Mass P. 898 –Nuclear Energy P. 902 –Radio Activity P. 906

VERY IMPORTANT:

Atomic Mass Unit, u One atomic mass unit (1 u) is equal to one- twelfth of the mass of the most abundant form of the carbon atom--carbon-12. Atomic mass unit: 1 u = x kg Common atomic masses: Proton: u Neutron: u Electron: uHydrogen: u

Example 1: The average atomic mass of Boron-11 is u. What is the mass of the nucleus of one boron atom in kg? Electron: u = The mass of the nucleus is the atomic mass less the mass of Z = 5 electrons: Mass = u – 5( u) 1 boron nucleus = u m = 1.83 x kg

Mass and Energy Recall Einstein’s equivalency formula for m and E: The energy of a mass of 1 u can be found: E = (1 u)c 2 = (1.66 x kg)(3 x 10 8 m/s) 2 E = 1.49 x J Or E = MeV When converting amu to energy:

Example 2: What is the rest mass energy of a proton ( u)? E = mc 2 = ( u)(931.5 MeV/u) Proton: E = MeV Similar conversions show other rest mass energies: Electron: E = MeV Neutron: E = MeV

The Mass Defect The mass defect is the difference between the rest mass of a nucleus and the sum of the rest masses of its constituent nucleons. The whole is less than the sum of the parts! Consider the carbon-12 atom ( u): Nuclear mass = Mass of atom – Electron masses = u – 6( u) = u The nucleus of the carbon-12 atom has this mass. (Continued...)

Mass Defect (Continued) Mass of carbon-12 nucleus: Proton: u Neutron: u The nucleus contains 6 protons and 6 neutrons: 6 p = 6( u) = u 6 n = 6( u) = u Total mass of parts: = u Mass defect m D = u – u m D = u

The Binding Energy The binding energy E B of a nucleus is the energy required to separate a nucleus into its constituent parts. E B = m D c 2 where c 2 = MeV/u The binding energy for the carbon-12 example is: E B = ( E B = ( u)(931.5 MeV/u) E B = 92.2 MeVBinding E B for C-12:

Binding Energy per Nucleon An important way of comparing the nuclei of atoms is finding their binding energy per nucleon: Binding energy per nucleon For our C-12 example A = 12 and:

Formula for Mass Defect The following formula is useful for mass defect: Mass defect m D m H = u; m n = u Z is atomic number; N is neutron number; M is mass of atom (including electrons). By using the mass of the hydrogen atom, you avoid the necessity of subtracting electron masses.

Example 3: Find the mass defect for the nucleus of helium-4. (M = u) Mass defect m D Zm H = (2)( u) = u Nm n = (2)( u) = u M = u (From nuclide tables) m D = ( u u) u m D = u

Example 3: Find the binding energy per nucleon for helium-4. (m D = u) E B = m D c 2 where c 2 = MeV/u E B = ( u)(931.5 MeV/u) = 28.3 MeV A total of 28.3 MeV is required To tear apart the nucleons from the He-4 atom. Since there are four nucleons, we find that

Binding Energy Vs. Mass Number Mass number A Binding Energy per nucleon Curve shows that E B increases with A and peaks at A = 60. Heavier nuclei are less stable. Green region is for most stable atoms. For heavier nuclei, energy is released when they break up (fission). For lighter nuclei, energy is released when they fuse together (fusion).

To do: P. 902 –Questions 1, 2 & 3