* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
Download Lecture 38
Survey
Document related concepts
Bremsstrahlung wikipedia , lookup
Photoelectric effect wikipedia , lookup
Auger electron spectroscopy wikipedia , lookup
X-ray photoelectron spectroscopy wikipedia , lookup
State of matter wikipedia , lookup
Heat transfer physics wikipedia , lookup
Two-dimensional nuclear magnetic resonance spectroscopy wikipedia , lookup
Atomic orbital wikipedia , lookup
Molecular Hamiltonian wikipedia , lookup
Degenerate matter wikipedia , lookup
Electron scattering wikipedia , lookup
Mössbauer spectroscopy wikipedia , lookup
Rutherford backscattering spectrometry wikipedia , lookup
Chemical bond wikipedia , lookup
Transcript
Summary Lecture 38 Electrons with the same n are in the same “shell”. Electrons with the same n and l are in the same “subshell”: l = 0 s- subshell, l = 1 p- subshell, l = 2 d- subshell. The exclusion principle limits the maximum number of electrons in each subshell to 2(2l + 1). Nucleus Radioactivity α-, β-, and γ- Decay Electron configurations are written by giving the value for n, the letter code for l, and the number of electrons in the subshell as a superscript. In some matter, atoms may have ionic or covalent bonding; potential-energy diagram shows how potential energy depends on the distance between atoms. Bond theory of matter divides all materials into conductors, semiconductors, and insulators. Conductors have high concentration of free electrons, insulators do not contain free electrons, and semiconductors have low concentration of free electrons. Semiconductors can be doped with some elements creating controlled free electrons or holes. Physics 112, Spring 2010, Apr 23, Lecture 38 Physics 112, Spring 2010, Apr 23, Lecture 38 Ionic Bonding Covalent Bonding Covalent bonding is caused by Ionic bonding is caused by 1) the transfer of electrons between atoms 2) the sharing of electrons between atoms 3) unequal charge distributions around neutral molecules 4) atoms bonding to hydrogen molecules 1) the transfer of electrons between atoms 2) the sharing of electrons between atoms 3) unequal charge distributions around neutral molecules 4) atoms bonding to hydrogen molecules A p-type Semiconductor An n-type Semiconductor A p-type semiconductor is produced by An n-type semiconductor is produced by 1) doping the host crystal with donor impurities 2) doping the host crystal with accepter impurities 3) pure crystals of germanium or silicone 4) none of the given answers 1) doping the host crystal with donor impurities 2) doping the host crystal with accepter impurities 3) pure crystals of germanium or silicone 4) none of the given answers Physics 112, Spring 2010, Apr 23, Lecture 38 2 3 Physics 112, Spring 2010, Apr 23, Lecture 38 4 1 Matter, Atom, Nucleus Structure of Nucleus Schematic representation of the structure of matter: Nucleus is made of nucleons: Electron + and Positive charge: q = 1.6 × 10 −19 C Matter + neutral + + mn = 1.67493×10−27 kg mp = 1.67262×10−27 kg + Atom Molecules or atoms Ratio (proton mass)/(electron mass): Each chemical element shown in the Periodic Table of Elements is build of electrons and nucleus with certain parameters. Carbon14 6 protons 8 neutrons (1.67262 × 10 −27 kg ) /(9.1× 10 −31 kg ) = 1838 + + + + + + Nucleus Nuclear matter is very dense: 5 Physics 112, Spring 2010, Apr 23, Lecture 38 Isotopes A Z Atomic number Z: the number of protons in a nucleus. Neutron number N: the number of neutrons in a nucleus. Nuclei of some atoms (e.g. carbon) contains the same number of protons but different number of neutrons (e.g. in carbon: 6 protons but 5,6,7, 8, or 10 neutrons). X Such nuclei are called isotopes. 11 6 C, 126C, 136C , 146C, Atomic mass number A = Z+N : the sum of protons and neutrons in nucleus. Atomic mass number “A” Atomic number “Z” 235 92 6 Physics 112, Spring 2010, Apr 23, Lecture 38 Nuclear Numerology and Symbols Nuclei are labeled by several numbers. ρ ≈ 1017 kg / m3 15 6 and 166C A Z X A=Z +N A is atomic mass number, Z atomic number (# of protons), N is the neutron number U Chemical symbol (name) 98.9% of naturally occurring carbon on Earth is the isotope 1.1% is the isotope 12 6 C 13 6 C These percentages are referred to as the natural abundances. Proton: 1 1 p Neutron: 1 0 n Electron: 0 −1 Some isotopes can be produced artificially. e The radius of nuclei: The protons carry positive charge: + The neutrons have no electrical charge: Physics 112, Spring 2010, Apr 23, Lecture 38 r ≈ (1.2 × 10 7 −15 The volume of nuclei: V∝A 4 3⎞ ⎛ ⎜V = π r ⎟ 3 ⎝ ⎠ Physics 112, Spring 2010, Apr 23, Lecture 38 8 1/ 3 m)( A ) 2 Comparison of Particles in Atom Binding Energy and Nuclear Forces (#1) Masses of atoms are measured with reference to the carbon-12 atom (6p+6n+6e), which is assigned a mass of exactly 12u. Binding energy: The total mass of a stable nucleus is always less than the sum of the masses of its separate protons and neutrons. 1 u = 1.6605 × 10 −27 kg “Unified atomic mass unit” (mass of 12C carbon is 12.000000 u). 6 E = mc2 = + Electron has a much smaller mass than a nucleon. Atomic mass unit can be specified using the electron-volt energy unit and eq. −27 + + + E = mc2 (1.67262×10 kg )(3 ×10 m / s) = 931.5 MeV 1.6 ×10−19 J / eV 8 2 + + Where has the missing mass gone? It has become energy, e.g. radiation or kinetic energy, released during the formation of the nucleus. Smaller total mass Binding energy of the nucleus = [mass of constituents - mass of the nucleus]c2 The strong nuclear, weak nuclear, electromagnetic and gravitational forces are the four known forces in nature. Strong nuclear force binds nucleons together. Weak nuclear force is responsible for radioactivity. 9 Physics 112, Spring 2010, Apr 23, Lecture 38 Binding Energy and Nuclear Forces (#2) 10 Physics 112, Spring 2010, Apr 23, Lecture 38 Radioactivity One feature of the nucleus is that number of neutrons ≈ number of protons. Radioactivity: Towards the end of the 19th century, minerals were found that would darken a photographic plate even in the absence of light. We can see this effect for stable nuclei with less than 20 protons. This phenomenon is now called radioactivity. There are 3 types of radioactive rays: Number of neutrons (N) Very large nuclei: no amount of extra neutrons can overcome the increasing Coulomb repulsion. Alpha rays (helium nuclei = 2 protons + 2 neutrons). Can barely penetrate a piece of paper. No stable nuclides for Z > 82. Bigger nuclei require extra neutrons (which only feel the strong force) to overcome the Coulomb repulsion of the extra protons. Beta rays (electrons (β-) or positrons (β+)). Can penetrate 3 mm of aluminum Gamma rays (high energy photons). Can penetrate several cm of lead Number of protons (Z) Physics 112, Spring 2010, Apr 23, Lecture 38 Unaffected by B field 11 Physics 112, Spring 2010, Apr 23, Lecture 38 α, β− are bent in opposite directions by B field. 12 3 Alpha Decay Beta Decay (#1) Alpha decay occurs in large nuclei when the Coulomb repulsion becomes so large that the strong nuclear force can no longer hold the nuclei together. Transmission of elements can occur when a nucleus decays beta decay: the emission of an electron or β- particle: Three types of decay: β-, β+, Electron capture (EC) For example, radium-226 will alpha-decay to radon-222: 226 88 4 222 Ra → 24 He + 222 86 X = 2 He + 86 Rn Here, the following reactions occur inside the nucleus. In general, alpha decay can be written: A Z + Alpha particle Unstable parent nucleus X→ A -4 Z-2 X + He ' 4 2 Total number of nucleons is unchanged) Daughter nucleus β- n → p + e− + υ β+ p → n + e+ + υ EC p + e → n +υ - Occurs when nucleus contains too many neutrons. Occurs when nucleus contains too many protons. υ is antineutrino. These reactions are governed by the weak nuclear force. 13 Physics 112, Spring 2010, Apr 23, Lecture 38 Physics 112, Spring 2010, Apr 23, Lecture 38 Beta Decay (#1) Beta Decay (#2) 2. Beta+ decay: Anti-neutrino 1. Beta- decay: p → n + e+ + υ − n → p + e + neutrino n → p + e− + υ Electron 19 10 Electron is created within the nucleus itself. Occurs when one of the neutrons in the nucleus changes into a proton. An electron and “antineutrino”υ are also ejected. Same number of nucleons, one more proton and one less neutron. A Z X A=Z +N 15 neutrino electron p + e- → n + υ 7 4 A is atomic mass number, Z atomic number (# of protons), N is the neutron number Physics 112, Spring 2010, Apr 23, Lecture 38 Ne → 199 F + e − + υ 3. Electron capture: Finally, a nucleus can capture one of its inner orbiting electrons. beta- decay of carbon-14: C → 147 N + e − + υ positron Occurs when one of the protons in the nucleus transforms into a neutron. A positron and neutrino are emitted. “Neutrino” means “little neutral one”; the symbol is nu (υ). 14 6 14 Be + e - → 73 Li + υ The electron is captured, a proton becomes a neutron and a neutrino is emitted. neutrino Physics 112, Spring 2010, Apr 23, Lecture 38 16 4 Gamma Decay Three Types of Radioactive Decay Gamma rays are very high-energy photons. They are emitted when a nucleus decays from an excited state to a lower state, just as photons are emitted by electrons returning to a lower state. Law of conservation of nucleon number: γ The total number of nucleons (A) remains constant in any process, although one type can change into the other type (protons into neutrons of vice versa). A Z X → ZA X + γ Physics 112, Spring 2010, Apr 23, Lecture 38 17 Physics 112, Spring 2010, Apr 23, Lecture 38 18 Mass of an Atom The mass of an atom is 1) approximately equally divided between neutrons, protons, and electrons 2) evenly divided between the nucleus and the surrounding electron cloud 3) concentrated in the cloud of electrons surrounding the nucleus 4) concentrated in the nucleus Atomic Number An atom's atomic number is determined by the number of 1) neutrons in its nucleus 2) nucleons in its nucleus 3) protons in its nucleus 4) alpha particles in its nucleus Physics 112, Spring 2010, Apr 23, Lecture 38 19 5