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About the Authors xiii
Foreword xv
Preface xvii
Acknowledgements xix
1 Basic Chemical and Biochemical Concepts 1
1.1 Chapter Overview 1
1.2 Energy and Chemical Reactions 1
1.3 Water and Hydrogen Bonds 15
1.4 Acids, Bases and pH 18
1.5 Summary of Key Concepts 25
2 Cells and their Basic Building Blocks 29
2.1 Chapter Overview 29
2.2 Lipids and Biomembranes 29
2.3 Carbohydrates and Sugars 32
2.4 Amino Acids, Polypeptides and Proteins 34
2.5 Nucleotides, Nucleic Acids, DNA, RNA and Genes 43
2.6 Cells and Pathogenic Bioparticles 51
2.7 Summary of Key Concepts 70
3 Basic Biophysical Concepts and Methods 73
3.1 Chapter Overview 73
3.2 Electrostatic Interactions 74
3.3 Hydrophobic and Hydration Forces 90
3.4 Osmolarity, Tonicity and Osmotic Pressure 91
3.5 Transport of Ions and Molecules across Cell Membranes 94
3.6 Electrochemical Gradients and Ion Distributions Across Membranes 99
3.7 Osmotic Properties of Cells 103
3.8 Probing the Electrical Properties of Cells 105
3.9 Membrane Equilibrium Potentials 111
3.10 Nernst Potential and Nernst Equation 112
3.11 The Equilibrium (Resting) Membrane Potential 114
3.12 Membrane Action Potential 116
3.13 Channel Conductance 120
3.14 The Voltage Clamp 121
3.15 Patch-Clamp Recording 122
3.16 Electrokinetic Effects 124
4 Spectroscopic Techniques 147
4.1 Chapter Overview 147
4.2 Introduction 148
4.3 Classes of Spectroscopy 151
4.4 The Beer-Lambert Law 165
4.5 Impedance Spectroscopy 170
5 Electrochemical Principles and Electrode Reactions 177
5.1 Chapter Overview 177
5.2 Introduction 178
5.3 Electrochemical Cells and Electrode Reactions 180
5.4 Electrical Control of Electron Transfer Reactions 194
5.5 Reference Electrodes 203
5.6 Electrochemical Impedance Spectroscopy (EIS) 208
6 Biosensors 215
6.1 Chapter Overview 215
6.2 Introduction 215
6.3 Immobilisation of the Biosensing Agent 217
6.4 Biosensor Parameters 218
6.5 Amperometric Biosensors 228
6.6 Potentiometric Biosensors 233
6.7 Conductometric and Impedimetric Biosensors 237
6.8 Sensors Based on Antibody-Antigen Interaction 240
6.9 Photometric Biosensors 242
6.10 Biomimetic Sensors 245
6.11 Glucose Sensors 247
6.12 Biocompatibility of Implantable Sensors 252
7 Basic Sensor Instrumentation and Electrochemical Sensor Interfaces 259
7.1 Chapter Overview 259
7.2 Transducer Basics 260
7.3 Sensor Amplification 262
7.4 The Operational Amplifier 264
7.5 Limitations of Operational Amplifiers 269
7.6 Instrumentation for Electrochemical Sensors 271
7.7 Impedance Based Biosensors 278
7.8 FET Based Biosensors 284
8 Instrumentation for Other Sensor Technologies 297
8.1 Chapter Overview 297
8.2 Temperature Sensors and Instrumentation 298
8.3 Mechanical Sensor Interfaces 304
8.4 Optical Biosensor Technology 325
8.5 Transducer Technology for Neuroscience and Medicine 335
9 Microfluidics: Basic Physics and Concepts 343
9.1 Chapter Overview 343
9.2 Liquids and Gases 343
9.3 Fluids Treated as a Continuum 346
9.4 Basic Fluidics 354
9.5 Fluid Dynamics 356
9.6 Navier-Stokes Equations 365
9.7 Continuum versus Molecular Model 369
9.8 Diffusion 378
9.9 Surface Tension 383
10 Microfluidics: Dimensional Analysis and Scaling 391
10.1 Chapter Overview 391
10.2 Dimensional Analysis 391
10.3 Dimensionless Parameters 400
10.4 Applying Nondimensional Parameters to Practical Flow Problems 411
10.5 Characteristic Time Scales 412
10.6 Applying Micro- and Nano-Physics to the Design of Microdevices 413
Problems 415
References 416
Appendix A: SI Prefixes 417
Appendix B: Values of Fundamental Physical Constants 419
Appendix C: Model Answers for Self-study Problems 421
Index 435
Chapter 2
Cells and their Basic Building Blocks
The chemical composition of a typical bacterium and animal (mammalian) cell is shown in Table 2.1.
Table 2.1 Approximate chemical composition of a typical bacterium and mammalian cell. (Adapted from Alberts et al. [1])
Leaving aside the water content of a cell, macromolecules such as proteins, nucleic acids (DNA, RNA), and polysaccharides make up a large percentage of a cell's mass. The building blocks for these macromolecules are small organic molecules, namely fatty acids, sugars, amino acids and nucleotides. This chapter describes the chemical structures and functions of these molecular building blocks, and the biological importance of the macromolecules and macrostructures they combine to form. A summary description is then given of how these macromolecules and microstructures interact and function in different types of cell.
After reading this chapter a basic understanding should be obtained of:
Cells of higher organisms are separated, but not isolated, from their surroundings by their cytoplasmic membrane, which also serves to act as anchors for proteins that transport or pump specific chemicals into or out of a cell. Membranes also define the boundaries of intracellular organelles and the nucleus in eukaryotic cells. The main structural components of biological membranes are lipids, which exist as derivatives of fatty acids. The term ‘lipid’ covers a wide range of molecules, including oils, waxes, sterols, certain (fat-soluble) vitamins and fats. The one property they all share in common is that they are hydrophobic. When placed in water individual lipid molecules will adopt a configuration that leads to minimum contact with water molecules, and will cluster into a group with other lipid molecules. This is exemplified by the formation of oil droplets in water, and how lipids in an aqueous medium segregate into a separate nonaqueous phase.
Fatty acid molecules contain a hydrocarbon chain, commonly consisting of 16 or 18 carbon atoms. An acidic carboxyl group (COOH) is attached to one end of this chain. Stearic acid CH3(CH2)16COOH and arachidic acid CH3(CH2)18COOH are examples, whose general chemical structure is shown below:
Stearic (n = 16) and arachidic (n = 18) acid are examples of fatty acids with no double (C=C) bonds in their hydrocarbon chain, and are termed as being saturated. If the hydrocarbon chain contains one or more double C=C bonds the fatty acid is termed unsaturated – an example of which is oleic acid CH3(CH2)7CH(CH2)7COOH:
The two hydrogen atoms attached to the carbons in the C=C double bond of oleic acid lie on the same side of the bond, and this configuration is known as the cis form. This cis configuration introduces a bend in the hydrocarbon chain. The other possible configuration, known as the trans form in which the two hydrogen atoms are situated on opposite sides of the C=C double bond, does not result in a bent hydrocarbon chain. The reason why butter and lard are solid at room temperature is because they are composed of saturated fatty acids whose straight hydrocarbon chains can pack closely together. Easily spreadable butter substitutes (e.g. margarine) contain unsaturated fatty acids that are unable to pack closely together because of the ‘kinks’ in their hydrocarbon chains, and have a softer form than butter at room temperature. Plant oils contain polyunsaturated fatty acids (with multiple C=C double bonds) and are liquid at room temperature.
A fatty acid molecule thus has two chemically distinct parts – a long hydrophobic chain that is not very reactive chemically, and a carboxyl group (COOH) which when ionised as COO− is chemically active and hydrophilic. Molecules such as these, which contain both hydrophobic and hydrophilic regions, are termed amphipathic. Fatty acids by themselves will not form a membrane that is capable of acting as a boundary between an aqueous medium and the aqueous cytoplasm of a cell. In aqueous media fatty acids will tend to form clusters, with the hydrocarbon chains packed together inside and the carboxylic acid groups directed outwards towards the surrounding water molecules. To form biomembranes fatty acids need to be converted into a structure that readily form sheets of lipid bilayers. The most common ones adopted in nature are phospholipids composed of two fatty acid side chains attached to a negatively charged (and hence hydrophilic) phosphate group via a glycerol molecule. The two fatty acid ‘tails’ may both be saturated, unsaturated, or adopt one of each form. As shown in Figure 2.1, in some phospholipids the ‘head’ of the molecule may be increased in size with the addition of an amine which can ionise to the hydrophilic form NH3+.
Figure 2.1 The chemical structure of a typical phospholipid (in this case phosphatidylethanolamine) to show its hydrophobic tail and hydrophilic head group.
Phospholipids can spontaneously form sheets of bilayers, two molecules thick, in an aqueous environment. As depicted in Figure 2.2, the hydrocarbon tails keep away from the water by aligning themselves in the middle of the bilayer structure. The close packing of the hydrocarbon tails is stabilised by van der Waals interactions, and the fluidity of the bilayer interior is influenced by the number of C=C double bonds in the hydrocarbon structures of the tails. The polar head groups are stabilised through hydrogen bonding to water molecules, as well as by electrostatic interactions between the phosphate and amine groups. As shown schematically in Figure 2.3 for a fat cell, the outer membrane of a cell is formed by a spherical lipid bilayer structure that encloses the cytoplasm and internal cell structures.
Figure 2.2 Schematic representation of a phospholipid bilayer. The small spheres represent the hydrophilic heads groups, and the lines are the hydrophobic hydrocarbon tails of individual phospholipid molecules.
Figure 2.3 Schematic representation of a fat cell (adipocyte).
Apart from their importance as precursors to phospholipids, fatty acids are used as a source of energy by tissues. Fat cells, known as adipocytes, contain one large droplet of lipid (see Figure 2.3). When triggered by hormones such as adrenaline these cells release fatty acids into their surrounding environment (normally blood), which are then broken down into smaller molecules identical to those derived from the breakdown of glucose.
Carbohydrates are composed of carbon atoms and the atoms that form water molecules, namely hydrogen and oxygen. Simple carbohydrates, called mono-saccharides, have the chemical structure (CH2O)n and are often referred to as simple sugars. The number ‘n’ of carbon atoms ranges from 3 to 7 and the corresponding sugar molecules are called trioses, tetroses, pentoses, hexoses and heptoses. We will learn later in this chapter that two pentose sugars (ribose and deoxyribose) are essential components of DNA and RNA. An important hexose is glucose (C6H12O6) because when it is broken down in cells of higher organisms it releases free energy. As shown in Figure 2.4 the linear structure of glucose can form a ring structure arising from the reaction of the aldehyde at the 1 carbon with the hydroxyl group on the 5 carbon, to form glucopyranose. A less common ring structure (glucofuranose) is formed by the reaction of the 1 carbon aldehyde with the hydroxyl on the 4 carbon. The chemical formula of a monosaccharide does not therefore fully describe the molecule. For example, a different sugar is formed if the hydrogen and hydroxyl groups attached to the 2 carbon of the D-glucose molecule switch places. This sugar (mannose) cannot be converted to glucose without breaking and making the relevant covalent bonds. Each of the sugars can also exist in either of two forms that are mirror images of each other, called the D-form...
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