Descriptive Inorganic Chemistry -  James E. House,  Kathleen A. House

Descriptive Inorganic Chemistry (eBook)

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2010 | 2. Auflage
592 Seiten
Elsevier Science (Verlag)
978-0-08-091677-4 (ISBN)
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This book covers the synthesis, reactions, and properties of elements and inorganic compounds ,for courses in descriptive inorganic chemistry. ,It is suitable for the one-semester (ACS-recommended) course or as a supplement in general chemistry courses. Ideal for major and non-majors, the book incorporates rich graphs and diagrams to enhance the content and maximize learning.

  • Includes expanded coverage of chemical bonding and enhanced treatment of Buckminster Fullerenes

  • Incorporates new industrial applications matched to key topics in the text

  • Descriptive Inorganic Chemistry, Second Edition, covers the synthesis, reactions, and properties of elements and inorganic compounds for courses in descriptive inorganic chemistry. This updated version includes expanded coverage of chemical bonding and enhanced treatment of Buckminster Fullerenes, and incorporates new industrial applications matched to key topics in the text. It is suitable for the one-semester (ACS-recommended) course or as a supplement in general chemistry courses. Ideal for majors and non-majors, the book incorporates rich graphs and diagrams to enhance the content and maximize learning. - Includes expanded coverage of chemical bonding and enhanced treatment of Buckminster Fullerenes- Incorporates new industrial applications matched to key topics in the text

    Front Cover 1
    Descriptive Inorganic Chemistry 4
    Copyright 5
    Table of Contents 6
    Preface 16
    Chapter 1. Where It All Comes From 18
    1.1 The Structure of the Earth 18
    1.2 Composition of the Earth’s Crust 21
    1.3 Rocks and Minerals 21
    1.4 Weathering 22
    1.5 Obtaining Metals 23
    1.6 Some Metals Today 27
    1.7 Nonmetallic Inorganic Minerals 29
    References for Further Reading 32
    Problems 32
    Chapter 2. Atomic and Molecular Structure 34
    2.1 Atomic Structure 34
    2.2 Properties of Atoms 40
    2.3 Molecular Structure 48
    2.4 Symmetry 61
    2.5 Resonance 68
    References for Further Reading 74
    Problems 74
    Chapter 3. Ionic Bonding, Crystals, and Intermolecular Forces 80
    3.1 Ionic Bonds 80
    3.2 Intermolecular Interactions 93
    References for Further Reading 105
    Problems 105
    Chapter 4. Reactions and Energy Relationships 108
    4.1 Thermodynamic Considerations 108
    4.2 Combination Reactions 120
    4.3 Decomposition Reactions 122
    4.4 Redox Reactions 124
    4.5 Hydrolysis Reactions 125
    4.6 Replacement Reactions 126
    4.7 Metathesis 127
    4.8 Neutralization Reactions 129
    References for Further Reading 131
    Problems 131
    Chapter 5. Acids, Bases, and Nonaqueous Solvents 136
    5.1 Acid-Base Chemistry 136
    5.2 Nonaqueous Solvents 153
    5.3 Superacids 165
    References for Further Reading 166
    Problems 166
    Chapter 6. Hydrogen 170
    6.1 Elemental and Positive Hydrogen 170
    6.2 Occurrence and Properties 175
    6.3 Hydrides 177
    References for Further Reading 183
    Problems 184
    Chapter 7. The Group IA and IIA Metals 186
    7.1 General Characteristics 187
    7.2 Oxides and Hydroxides 192
    7.3 Halides 195
    7.4 Sulfides 196
    7.5 Nitrides and Phosphides 197
    7.6 Carbides, Cyanides, Cyanamides, and Amides 198
    7.7 Carbonates, Nitrates, Sulfates, and Phosphates 199
    7.8 Organic Derivatives 200
    References for Further Reading 203
    Problems 204
    Chapter 8. Boron 206
    8.1 Elemental Boron 206
    8.2 Bonding in Boron Compounds 208
    8.3 Boron Compounds 208
    References for Further Reading 220
    Problems 221
    Chapter 9. Aluminum, Gallium, Indium, and Thallium 224
    9.1 The Elements 224
    9.2 Oxides 228
    9.3 Hydrides 231
    9.4 Halides 232
    9.5 Other Compounds 234
    9.6 Organometallic Compounds 236
    References for Further Reading 239
    Problems 239
    Chapter 10. Carbon 242
    10.1 The Element 242
    10.2 Industrial Uses of Carbon 246
    10.3 Carbon Compounds 248
    10.4 Fullerenes 259
    References for Further Reading 260
    Problems 261
    Chapter 11. Silicon, Germanium, Tin, and Lead 264
    11.1 The Elements 264
    11.2 Hydrides of the Group IVA Elements 268
    11.3 Oxides of the Group IVA Elements 269
    11.4 Silicates 275
    11.5 Zeolites 280
    11.6 Halides of the Group IVA Elements 282
    11.7 Organic Compounds 286
    11.8 Miscellaneous Compounds 288
    References for Further Reading 290
    Problems 291
    Chapter 12. Nitrogen 294
    12.1 Elemental Nitrogen 294
    12.2 Nitrides 295
    12.3 Ammonia and Aquo Compounds 296
    12.4 Hydrogen Compounds 297
    12.5 Nitrogen Halides 303
    12.6 Nitrogen Oxides 305
    12.7 Oxyacids 310
    References for Further Reading 314
    Problems 314
    Chapter 13. Phosphorus, Arsenic, Antimony, and Bismuth 318
    13.1 Occurrence 318
    13.2 Preparation and Properties of the Elements 319
    13.3 Hydrides 320
    13.4 Oxides 322
    13.5 Sulfides 324
    13.6 Halides 325
    13.7 Phosphonitrilic Compounds 332
    13.8 Acids and Their Salts 334
    13.9 Fertilizer Production 340
    References for Further Reading 342
    Problems 343
    Chapter 14. Oxygen 346
    14.1 Elemental Oxygen, O2 346
    14.2 Ozone, O3 348
    14.3 Preparation of Oxygen 350
    14.4 Binary Compounds of Oxygen 350
    14.5 Positive Oxygen 355
    References for Further Reading 356
    Problems 356
    Chapter 15. Sulfur, Selenium, and Tellurium 358
    15.1 Occurrence of Sulfur 358
    15.2 Occurrence of Selenium and Tellurium 360
    15.3 Elemental Sulfur 361
    15.4 Elemental Selenium and Tellurium 363
    15.5 Reactions of Elemental Selenium and Tellurium 364
    15.6 Hydrogen Compounds 365
    15.7 Oxides of Sulfur, Selenium, and Tellurium 367
    15.8 Halogen Compounds 370
    15.9 Nitrogen Compounds 373
    15.10 Oxyhalides of Sulfur and Selenium 376
    15.11 Oxyacids of Sulfur, Selenium, and Tellurium 379
    15.12 Sulfuric Acid 384
    References for Further Reading 389
    Problems 389
    Chapter 16. Halogens 392
    16.1 Occurrence 392
    16.2 The Elements 393
    16.3 Interhalogens 395
    16.4 Polyatomic Cations and Anions 401
    16.5 Hydrogen Halides 404
    16.6 Oxides 406
    16.7 Oxyacids and Oxyanions 411
    References for Further Reading 415
    Problems 415
    Chapter 17. The Noble Gases 418
    17.1 The Elements 418
    17.2 The Xenon Fluorides 421
    17.3 Reactions of Xenon Fluorides 424
    17.4 Oxyfluorides and Oxides 426
    References for Further Reading 427
    Problems 428
    Chapter 18. The Transition Metals 430
    18.1 The Metals 430
    18.2 Oxides 441
    18.3 Halides and Oxyhalides 447
    18.4 Miscellaneous Compounds 449
    18.5 The Lanthanides 451
    References for Further Reading 454
    Problems 454
    Chapter 19. Structure and Bonding in Coordination Compounds 458
    19.1 Types of Ligands and Complexes 458
    19.2 Naming Coordination Compounds 461
    19.3 Isomerism 463
    19.4 Factors Affecting the Stability of Complexes 468
    19.5 A Valence Bond Approach to Bonding in Complexes 472
    19.6 Back Donation 478
    19.7 Ligand Field Theory 481
    19.8 Jahn-Teller Distortion 490
    References for Further Reading 491
    Problems 492
    Chapter 20. Synthesis and Reactions of Coordination Compounds 496
    20.1 Synthesis of Coordination Compounds 496
    20.2 A Survey of Reaction Types 501
    20.3 A Closer Look at Substitution Reactions 510
    20.4 Substitution in Square Planar Complexes 513
    20.5 Substitution in Octahedral Complexes 522
    References for Further Reading 528
    Problems 529
    Chapter 21. Organometallic Compounds 534
    21.1 Structure and Bonding in Metal Alkyls 535
    21.2 Preparation of Organometallic Compounds 539
    21.3 Reactions of Metal Alkyls 542
    21.4 Cyclopentadienyl Complexes (Metallocenes) 545
    21.5 Metal Carbonyl Complexes 548
    21.6 Metal Olefin Complexes 558
    21.7 Complexes of Benzene and Related Aromatics 562
    References for Further Reading 563
    Problems 564
    Appendix A. Ground State Electron Configurations of Atoms 568
    Appendix B. Ionization Energies 572
    Index 576

    CHAPTER 2

    Atomic and Molecular Structure


    Because so much of the chemistry of atoms and molecules is related to their structures, the study of descriptive chemistry begins with a consideration of these topics. The reasons for this are simple and straightforward. For example, many of the chemical characteristics of nitrogen are attributable to the structure of the N2 molecule, :N ≡ N:. The triple bond in the N2 molecule is very strong, and that bond strength is responsible for many chemical properties of nitrogen (such as it being a relatively unreactive gas). Likewise, to understand the basis for the enormous difference in the chemical behavior of SF4 and SF6 it is necessary to understand the difference between the structures of these molecules, which can be shown as


    Moreover, to understand why SF6 exists as a stable compound whereas SCl6 does not, we need to know something about the properties of the S, F, and Cl atoms. As another illustration, it may be asked why the PO43− ion is quite stable but NO43− is not. Throughout this descriptive chemistry book, reference will be made in many instances to differences in chemical behavior that are based on atomic and molecular properties. Certainly not all chemical characteristics are predictable from an understanding of atomic and molecular structure. However, structural principles are useful in so many cases (for both comprehension of facts and prediction of properties) that a study of atomic and molecular structure is essential.

    What follows is a nonmathematical treatment of the aspects of atomic and molecular structure that provides an adequate basis for understanding much of the chemistry presented later in this book. Much of this chapter should be a review of principles learned in earlier chemistry courses, which is intentional. More theoretical treatments of these topics can be found in the suggested readings at the end of this chapter.

    2.1 Atomic Structure


    A knowledge of the structure of atoms provides the basis for understanding how they combine and the types of bonds that are formed. In this section, we review early work in this area, and variations in atomic properties will be related to the periodic table.

    2.1.1 Quantum Numbers


    It was the analysis of the line spectrum of hydrogen observed by J. J. Balmer and others that led Neils Bohr to a treatment of the hydrogen atom that is now referred to as the Bohr model. In that model, there are supposedly “allowed” orbits in which the electron can move around the nucleus without radiating electromagnetic energy. The orbits are those for which the angular momentum, mvr, can have only certain values (they are referred to as quantized). This condition can be represented by the relationship

    vr=nh2π (2.1)

    (2.1)

    where n is an integer (1, 2, 3, …) corresponding to the orbit, h is Planck’s constant, m is the mass of the electron, v is its velocity, and r is the radius of the orbit. Although the Bohr model gave a successful interpretation of the line spectrum of hydrogen, it did not explain the spectral properties of species other than hydrogen and ions containing a single electron (He+, Li2+, etc.).

    In 1924, Louis de Broglie, as a young doctoral student, investigated some of the consequences of relativity theory. It was known that for electromagnetic radiation, the energy, E, is expressed by the Planck relationship,

    =hυ=hcλ (2.2)

    (2.2)

    where c, ν, and λ are the velocity, frequency, and wavelength of the radiation, respectively. The photon also has an energy given by a relationship obtained from relativity theory,

    =mc2 (2.3)

    (2.3)

    A specific photon can have only one energy, so the right-hand sides of Eqs. (2.2) and (2.3) must be equal. Therefore,

    cλ=mc2 (2.4)

    (2.4)

    and solving for the wavelength gives

    =hmc (2.5)

    (2.5)

    The product of mass and velocity equals momentum, so the wavelength of a photon, represented by h/mc, is Planck’s constant divided by its momentum. Because particles have many of the characteristics of photons, de Broglie reasoned that for a particle moving at a velocity, ν, there should be an associated wavelength that is expressed as

    =hmv (2.6)

    (2.6)

    This predicted wave character was verified in 1927 by C. J. Davisson and L. H. Germer who studied the diffraction of an electron beam that was directed at a nickel crystal. Diffraction is a characteristic of waves, so it was demonstrated that moving electrons have a wave character.

    If an electron behaves as a wave as it moves in a hydrogen atom, a stable orbit can result only when the circumference of a circular orbit contains a whole number of waves. In that way, the waves can join smoothly to produce a standing wave with the circumference being equal to an integral number of wavelengths. This equality can be represented as

    πr=nλ (2.7)

    (2.7)

    where n is an integer. Because λ is equal to h/mv, substitution of this value in Eq. (2.7) gives

    πr=nhmv (2.8)

    (2.8)

    which can be rearranged to give

    vr=nh2π (2.9)

    (2.9)

    It should be noted that this relationship is identical to Bohr’s assumption about stable orbits (shown in Eq. 2.1)!

    In 1926, Erwin Schrödinger made use of the wave character of the electron and adapted a previously known equation for three-dimensional waves to the hydrogen atom problem. The result is known as the Schrödinger wave equation for the hydrogen atom, which can be written as

    2Ψ+2mℏ2(E−V)Ψ=0 (2.10)

    (2.10)

    where Ψ is the wave function, ħ is h/2π, m is the mass of the electron, E is the total energy, V is the potential energy (in this case the electrostatic energy) of the system, and ∇2 is the Laplacian operator:

    2=∂2∂x2+∂2∂y2+∂2∂z2 (2.11)

    (2.11)

    The wave function is, therefore, a function of the coordinates of the parts of the system that completely describes the system. A useful characteristic of the quantum mechanical way of treating problems is that once the wave function is known, it provides a way for calculating some properties of the system.

    The Schrödinger equation for the hydrogen atom is a second-order partial differential equation in three variables. A customary technique for solving this type of differential equation is by a procedure known as the separation of variables. In that way, a complicated equation that contains multiple variables is reduced to multiple equations, each of which contains a smaller number of variables. The potential energy, V, is a function of the distance of the electron from the nucleus, and this distance is represented in Cartesian coordinates as r = (x2 + y2 + z2)1/2. Because of this relationship, it is impossible to use the separation of variables technique. Schrödinger solved the wave equation by first transforming the Laplacian operator into polar coordinates. The resulting equation can be written as

    r2∂∂rr2∂Ψ∂r+1r2sinθ∂∂θ(sinθ∂Ψ∂θ)+1r2sin2θ∂2Ψ∂φ2+2mℏ2(E+e2r)Ψ=0 (2.12)

    (2.12)

    Although no attempt will be made to solve this very complicated equation, it should be pointed out that in this form the separation of the variables is possible, and equations that are functions of r, θ, and ϕ result. Each of the simpler equations that are obtained can be solved to give solutions that are functions of only one variable. These partial solutions are described by the functions R(r), Θ(θ), and Φ(ϕ), respectively, and the overall solution is the product of these partial solutions.

    It is important to note at this point that the mathematical restrictions imposed by solving the differential equations naturally lead to some restraints on the nature of the solutions. For example, solution of the equation containing r requires the introduction of an integer, n, which can have the values n = 1, 2, 3, … and an integer l, which has values that are related to the value of n such that l = 0, 1, 2, … (n − 1). For a given value of n, the values for l can be all integers from 0 up to (n − 1). The quantum number n is called the principal quantum number and l is called the angular momentum quantum number. The principal quantum number determines the energy of the state for the hydrogen atom, but for complex atoms the energy also depends on l.

    The partial solution of the equation that contains the angular dependence results in the introduction of another quantum number, ml. This number is called the magnetic quantum...

    Erscheint lt. Verlag 22.9.2010
    Sprache englisch
    Themenwelt Naturwissenschaften Chemie Anorganische Chemie
    Technik
    ISBN-10 0-08-091677-5 / 0080916775
    ISBN-13 978-0-08-091677-4 / 9780080916774
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