1 / 49

: Atomic Systems and Bonding :

: Atomic Systems and Bonding :. R. R. Lindeke, Ph.D. ME 2105– Lecture Series 2. ISSUES TO ADDRESS. The Structure of Matter A Quick Review from chemistry What Promotes Bonding? What type of Bonding is Possible? What Properties are Inferred from Bonding?. How the atoms are arranged

lotta
Download Presentation

: Atomic Systems and Bonding :

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. : Atomic Systems and Bonding : R. R. Lindeke, Ph.D. ME 2105– Lecture Series 2

  2. ISSUES TO ADDRESS... • The Structure of Matter • A Quick Review from chemistry • What Promotes Bonding? • What type of Bonding is Possible? • What Properties are Inferred from Bonding?

  3. How the atoms are arranged & how they bond GREATLY AFFECTS Their FINAL PROPERTIES & therefore use ATOMIC Structure Electron configurations Primary & secondary BONDING Just as before:

  4. Structure of Matter: • Atoms are the smallest particle in Nature that exhibits the characteristics of a substance • The radius of a typical atom is on the order of 0. 0.0000000001 meter and cannot be studied without very powerful microscopes Pictured here is an “Electron Microscope” It can greatly magnify materials but can’t resolve individual atom – we need a TEM or STP for that

  5. Structure of Matter: A molecule consists of 2 or more atoms bound together In a common glass of water “upon closer examination” we would find a huge number of Water “Molecules” consisting of 1 atom of Oxygen and 2 atoms of hydrogen

  6. Atomic Structure (Freshman Chem.) (.000911x 10-27 kg) • atom –electrons– 9.11 x 10-31 kgprotonsneutrons • atomic number = # of protons in nucleus of atom = # of electrons of neutral species • A [=] atomic mass unit = amu = 1/12 mass of 12CAtomic wt = wt of 6.023 x 1023 molecules or atoms 1 amu/atom = 1g/mol C 12.011 H 1.008 etc. } 1.67 x 10-27 kg Atomic Weight is rarely a whole number – it is a weighted average of all of the natural isotopes of an “Element”

  7. What is this in weight or mass in “Real Terms” • Example 1:

  8. What is this in weight or mass in “Real Terms”

  9. Structure of Matter – an Element • Any material that is composed of only one type of atom is called a chemical element, a basic element, or just an element. • Every element has a unique atomic structure. • Scientists know of only about 109 basic elements at this time. (This number has a habit of changing!) • All matter is composed of combinations of one or more of these elements. • Ninety-one of these basic elements occur naturally on or in the Earth (Hydrogen to Uraninum). • These elements are pictured in the “Periodic Table”

  10. The Periodic Table of the Elements

  11. Structure of Matter • Each of the “boxes” in the periodic table help us to understand the details of a given elements • Here we see atomic Number (# of Electrons or Protons) and Atomic Weight • Some tables provide information about an elements “Valance State” or the ability to gain or shed their outermost electrons when they form molecules or “Compounds”

  12. Structure of Matter • These outermost or Valence electrons determine all of the following properties concerning an element: • Chemical • Electrical • Thermal • Optical

  13. Schematic Image of Atoms: Atomic number is 29

  14. Electronic Structure • Electrons have wavelike and particulate properties. • This means that electrons exist in orbitals defined by a probability. – Boer coupled w/ Schrödinger models • Each orbital is located at a discrete energy level determined by quantum numbers. Quantum #Designation n = principal (energy level/shell) K, L, M, N, O (1, 2, 3, etc.) l = subsidiary (orbitals) s, p, d, f (0, 1, 2, 3,…, n-1) ml = magnetic 1(s), 3(p), 5(d), 7(f) ms = spin ½, -½

  15. 4d N-shell n = 4 4p 3d 4s 3p M-shell n = 3 Energy 3s 2p L-shell n = 2 2s 1s K-shell n = 1 Electron Energy States • have discrete energy states • tend to occupy lowest available energy state. Electrons Can hold up to 32 electrons Can hold up to 18 Electrons Can hold up to 8 electrons Can hold up to 2 electrons Adapted from Fig. 2.4, Callister 7e.

  16. More exhaustively:

  17. SURVEY OF ELEMENTS Element Atomic # Electron configuration Hydrogen 1 1s 1 Helium 2 (stable) 1s 2 Lithium 3 1s 2 2s 1 Beryllium 4 1s 2 2s 2 Boron 5 1s 2 2s 2 2p 1 1s 2 2s 2 2p 2 Carbon 6 ... ... Neon 10 1s 2 2s 2 2p 6 (stable) Sodium 11 1s 2 2s 2 2p 6 3s 1 1s 2 2s 2 2p 6 3s 2 Magnesium 12 1s 2 2s 2 2p 6 3s 2 3p 1 Aluminum 13 ... ... 1s 2 2s 2 2p 6 3s 2 3p 6 (stable) Argon 18 ... ... ... Krypton 36 1s 2 2s 2 2p 6 3s 2 3p 6 3d 10 4s 2 4p 6 (stable) • For Most elements: This Electron configuration not stable. • Why? Valence (outer) shell usually not filled completely so the electrons can ‘move out’!

  18. 1s2 2s2 2p6 3s2 3p6 3d6 4s2 ex: Fe - atomic # = 4d N-shell n = 4 4p 3d 4s 3p M-shell n = 3 Energy 3s 2p L-shell n = 2 2s 1s K-shell n = 1 Lets Try one: Here we have Iron ‘Fe’ (w/ Atomic Number 26)

  19. valence electrons Electron Configurations • Valence electrons – those in unfilled shells • Filled shells are more stable • Valence electrons are most available for bonding and tend to control the chemical properties • example: C (atomic number = 6) 1s22s2 2p2

  20. inert gases give up 1e give up 2e accept 2e accept 1e give up 3e H He Li Be O F Ne Na Mg S Cl Ar K Ca Sc Se Br Kr Rb Sr Y Te I Xe Cs Ba Po At Rn Fr Ra Matter (or elements) Bond as a result of their Valance states Electropositive elements: Readily give up electrons to become + ions. Electronegative elements: Readily acquire electrons to become - ions.

  21. Molecular/Elemental Bonding • Bonding is the result of the balance of the force of attraction and the force of repulsion of the electric nature of atoms (ions) • Net Force between atoms: FN = FA + FR and at some equilibrium (stable) bond location of separation, FN = 0 or FA = FR • From Physics we like to talk about bonding energy where:

  22. A B EN = EA+ ER = - - r r n Repulsive energy ER Interatomic separation r Net energy EN Attractive energy EA Bonding Energy Equilibrium separation (r0) is about .3 nm for many atoms • Energy – minimum energy most stable • Energy balance of attractive and repulsive terms n is 7-9 for most ionic pairs

  23. A B EN = EA+ ER = - - r r n Here: A, B and n are “material constants”

  24. Figure 2.7 Net bonding force curve for a Na+−Cl− pair showing an equilibrium bond length of a0 = 0.28 nm.

  25. Bonding Energy, the Curve Shape, and Bonding Type • Properties depend on shape, bonding type and values of curves: they vary for different materials. • Bonding energy (minimum on curve) is the energy that would be required to separate the two atoms to an infinite separation. • Modulus of elasticity depends on energy (force) versus distance curve: the slope at r = r0 position on the curve will be quite steep for very stiff materials, slopes are shallower for more flexible materials. • Coefficient of thermal expansion depends on E0 versus r0 curve: a deep and narrow trough correlates with a low coefficient of thermal expansion

  26. Bonding Types of Interest: • Ionic Bonding: Based on donation and acceptance of valance electrons between elements to create strong “ions” – CaIONs and AnIONs due to large electro-negativity differences • Covalent Bonding: Based on the ‘sharing’ of valance electrons due to small electro negativity differences • Metallic Bonding: All free electrons act as a moving ‘cloud’ or ‘sea’ to keep charged ion cores from flying apart in their ‘stable’ structure • secondary bonding: van der wahl’s attractive forces between molecules (with + to – ‘ends’) • This system of attraction takes place without valance electron participation in the whole • Valence Electrons participate in the bonding to build the molecules not in ‘gluing’ the molecules together

  27. Ionic bond – metal + nonmetal donates accepts electrons electrons Dissimilar electronegativities   ex: MgOMg 1s2 2s2 2p63s2O 1s2 2s2 2p4 [Ne] 3s2 Mg2+1s2 2s2 2p6O2- 1s2 2s2 2p6 [Ne] [Ne] Note: after exchange we have a stable (albeit ionic) electron structure for both Mg & O!

  28. Examples: Ionic Bonding NaCl MgO CaF 2 CsCl Give up electrons Acquire electrons • Predominant bonding in Ceramics

  29. Ionic Bonding – a Closely held Structure of +Ions and –Ions (after this Valence exchange) • These structure a held together by Coulombic Bonding forces after the Atoms exchange Valance Electrons to form the stable ionic cores: • It the solid state these ionic cores will sit at highly structured “Crystallographic Sites” • We can compute the coulombic forces holding the ions together – it is a balance between attraction force (energy) due to the ionic charge and repulsion force (energy) due to the nuclear cores of the ions • These forces of attraction and repulsion compete and will achieve a energy minimum at some inter-ion spacing

  30. Figure 2.10Formation of an ionic bond note effect of ionization on atomic radius. The cation (Na+) becomes smaller than the neutral atom, while the anion (Cl−) becomes larger than the neutral atom

  31. Example: Using these energy issues Here, ‘r0’equals the sum of the ionic radii of each and represents the r in the energy balance equations!

  32. Another Example (working backward with Coulomb’s Law):

  33. The largest number of ions of radius R that can coordinate an atom of radius r is 3 when the radius ratio r/R = 0.2. (Note: The instability for CN = 4 can be reduced, but not eliminated, by allowing a three-dimensional, rather than a coplanar, stacking of the larger ions.) – to keep the ionic characteristic in balance!

  34. The minimum radius ratio, r/R, that can produce threefold coordination is 0.155

  35. Covalent Bonding shared electrons H C: has 4 valence e-, needs 4 more from carbon atom CH 4 H: has 1 valence e-, needs 1 more H H C shared electrons Electronegativities are comparable. from hydrogen H atoms Adapted from Fig. 2.10, Callister 7e. • similar electronegativity share electrons • bonds determined by valence – s & p orbitals dominate bonding • Example: CH4

  36. Three-dimensional structure of bonding in the covalent solid, carbon (diamond). Each carbon atom (C) has four covalent bonds to four other carbon atoms. Note, the bond-line schematic of covalent bonding is given a perspective view to emphasize the spatial arrangement of bonded carbon atoms.

  37. Tetrahedral configuration of covalent bonds with carbon. The bond angle is 109.5°.

  38. During Polymerization, We break up one “double bond” (must supply 162 kcal/mole) and add two single bonds (releases 2*88 = 176 kcal/mole) which requires a catalyst to start but will be self-sustaining (releasing heat!) once the process begins

  39. Give up electrons Acquire electrons “Electro-negativity” Values for determining Ionic vs. Covalent Bond Character

  40. x ( 100 %) Primary Bonding Ionic-Covalent Mixed Bonding % ionic character = where XA & XB are ‘Pauling’ electronegativities Ex: MgO XMg = 1.2XO = 3.5

  41. Metallic Bonding: In a metallic bonded material, the valence electrons are “shared” among all of the ionic cores in the structure not just with nearest neighbors!

  42. Considering Copper: • It valance electrons are far from the nucleus and thus are not too tightly bound (making it easier to ‘move out’) • outside shell had only one electron • When the valence electron in any atom gains sufficient energy from some outside force, it can break away from the parent atom and become what is called a free electron • Atoms with few electrons in their valence shell tend to have more free electrons since these valence electrons are more loosely bound to the nucleus. In some materials like copper, the electrons are so loosely held by the atom and so close to the neighboring atoms that it is difficult to determine which electron belongs to which atom! • Under normal conditions the movement of the electrons is truly random, meaning they are moving in all directions by the same amount. • However, if some outside force acts upon the material, this flow of electrons can be directed through materials and this flow is called electrical current in a conductor.

  43. SECONDARY BONDING • Fluctuating dipoles ex: liquid H 2 asymmetric electron H H 2 2 clouds + - + - H H H H secondary secondary bonding Adapted from Fig. 2.13, Callister 7e. bonding secondary -general case: + - + - bonding Adapted from Fig. 2.14, Callister 7e. secondary -ex: liquid HCl Cl Cl H H bonding secondary bonding -ex: polymer secondary bonding Arises from interaction between “electric” dipoles • Permanent dipoles-molecule induced

  44. Summary: Bonding Comments Type Bond Energy Ionic Large! Nondirectional (ceramics) Directional (semiconductors, ceramics polymer chains) Covalent Variable large-Diamond small-Bismuth Metallic Variable large-Tungsten Nondirectional (metals) small-Mercury Secondary smallest Directional inter-chain (polymer) inter-molecular

  45. Properties From Bonding: Tm Energy r r o r Energy smaller Tm unstretched length larger Tm r o r Eo = “bond energy” • Melting Temperature, Tm • Bond length, r • Bond energy, Eo Tm is larger if Eo is larger.

  46. Properties From Bonding : a length, L o unheated, T 1 D L heated, T 2 r o Energy unstretched length r smaller a Eo Eo larger a • Coefficient of thermal expansion, a coeff. thermal expansion D L a = ( T - T ) 2 1 • a ~ symmetry at ro L o a is larger if Eo is smaller.

  47. Summary: Primary Bonds secondary bonding Large bond energy large Tm large E small a Ceramics (Ionic & covalent bonding): Metals Variable bond energy moderate Tm moderate E moderate a (Metallic bonding): Polymers Directional Properties Secondary bonding dominates small Tm small E large a (Covalent & Secondary):

More Related