| Chapter 1: Atoms – knowledge statements and learning goals |
In 1963, Nobel Laureate Richard Feynman (1918-1988), one of the most accomplished and influential scientists of the 20th century, wrote: “If, in some cataclysm, all of scientific knowledge were to be destroyed, and only one sentence passed on to the next generation of creatures, what statement would contain the most information in the fewest words? I believe it is the atomic hypothesis (or the atomic fact, or whatever you wish to call it) that all things are made of atoms—little particles that move around in perpetual motion, attracting each other when they are a little distance apart, but repelling on being squeezed into one another. In that one sentence, you will see, there is an enormous amount of information about the world, if just a little imagination and thinking are applied.” (Feynman 1963) |
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Most of us are quite familiar with the idea that matter is composed of atoms, we have been told that this is so since childhood. But how many of us really (and we mean really) believe it, or know the reasons that it is assumed to be true? It seems so completely and totally impossible (and improbable) - we do not experience atoms directly, and it is easy to go through life, quite successfully for the vast majority of us, without having to take atoms seriously. |
It seems so completely and totally impossible (and improbable) - we do not experience atoms directly, and it is easy to go through life, quite successfully for the vast majority of us, without having to take atoms seriously. Atomic Theory is also critical for understanding a significant number of the underlying concepts of biology and physics, not to mention geology, astronomy, ecology, and engineering. How can one sentence contain so much information? Can we really explain such a vast and diverse set of scientific observations with so little to go on? In the next two chapters we will expand on Feynman’s sentence to see just what you can do with a little “imagination and thinking”. At the same time, it is worth remembering that the fact that atoms are so unreal, from the perspective of our day to day experience, means that the atomic hypothesis poses a serious barrier to understanding modern chemistry. This is a barrier that can only be dealt with if you recognize it explicitly, and try to address and adjust to it – you will be rewiring your brain in order to take atoms, and all that they imply, seriously. We are aware that this is not an easy task. It takes effort, and much of this effort will involve self-reflection, problem-solving, and question answering. In an important sense, you do not have to believe in atoms, but you do have to understand them. What do you think you know about atoms: Current theory holds that atoms consist of a very (very) small, but very dense nucleus that contains protons and neutrons, which is surrounded by electrons, which are very light, relatively. The space occupied by moving electrons accounts for the vast majority of the volume of an atom. Because the number of positively charged protons and negatively charged electrons are equal, and the size of the charges are the same (but opposite), atoms are electrically neutral when taken as a whole, that is: each positively charged proton is counterbalanced by a negatively charged electron. Often the definition of an atom contains some language about how atoms have the same chemical properties of an element, but what do we mean by chemical properties? Can an atom have chemical properties? And how can ensembles of the same particles (protons, electrons, and neutrons) have different properties – this is the mystery of the atom, and understanding it is the foundation of chemistry. In this first chapter we will (hopefully) lead you to a basic understanding of atomic structure and inter-atomic interactions. Subsequent chapters will extend and deepen this understanding. |
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Atomic Realities The full story of how we know what we know about the existence and structure of atoms is fascinating, complex and, perhaps fortunately for you, too long to go into complete detail here. This is partially because much of it is considered physics - although in fact where physics ends and chemistry begins is rather arbitrary. What we do want to do is to consider a number of key points that illustrate how our ideas of atoms arose and have changed over time. We will present the evidence that has made accepting the atomic theory unavoidable if you want to explain, and manipulate, chemical reactions and the behavior of matter. Atomic theory is an example of a scientific theory that began as speculation and, through the constraints provided by careful observation, experimentation, and logical consistency, evolved over time into a detailed set of ideas that made accurate predictions and was able to explain an increasing number of diverse, and often previously unknown, phenomena. As new observations were made and became well established, atomic theory was adapted to accommodate and organize them. A key feature of scientific, as opposed to other types of ideas, is not whether they are right or wrong, but whether they are logically coherent and make unambiguous, observable, and generally quantitative predictions. They tell us what to look for and what we will find if we measure it. When we look, we may find the world to be as predicted (confirmation of the ideas) or something different. If the world is different from what our scientific ideas suggest, then we assume we are missing something important - either our ideas need altering, or perhaps we are not looking at the world in the right way. As we will see, the types of observations and experimental evidence about matter have become increasingly accurate, complex, and often abstract (that is, not part of our immediate experience). Some of it can be quite difficult to understand, since matter behaves quite differently on the atomic and sub-atomic (microscopic) scale than it does in the normal (macroscopic) world. It is the macroscopic world that evolutionary processes have adapted us to understand (or at least cope with) and with which we are familiar. Yet, if we are to be scientific, we have to go where the data leads us. If we obtain results that are not consistent with our intuitions and current theories, we have to revise those theories rather than ignore the data. However, scientists tend to be conservative in revising well established theories because new data can sometimes be misleading; this is one reason there is so much emphasis placed on reproducibility. A single report, no matter how careful it appears, can be wrong; the ability of other scientists to reproduce the observation/experiment is key to its acceptance (this is why there are no “miracles” in science.) Even then, the meaning of an observation is not always obvious or unambiguous; more often than not a "revolutionary observation" has a prosaic, that is simple, unrevolutionary, and often boring explanation. Truly revolutionary observations are few and far between (and one might argue, getting rarer as we approach an increasingly complete scientific understanding of the world in which we live.[optional link]) This is one reason that the oft quoted statement by Carl Sagan is oft quoted: "Extraordinary claims require extraordinary evidence." In many cases where revolutionary data is reported, subsequent studies often find that results are due to poor experimental design, sloppiness, or irrelevant factors - the fact that we all do not have cold fusion energy plants driving perpetual motion refrigerators in our homes is evidence of that. A common misconception about scientific theories is that they are simply “ideas” that someone came up with on the spur of the moment. In everyday use, the word “theory” may well mean an idea or even a hypothesis or working assumption, but in science the word theory should be (but often isn't) reserved for explanations that encompass and explain a broad range of observations. More than just an explanation, however, a theory must be well tested and make clear predictions relating to new observations or experiments. For example, the theory of evolution predicts that when one looks at the fossil record one will find evidence for animals that share many of the features of modern humans. This is a prediction made before any such fossils were found; in fact, many fossils of human-like organisms have, and continue to be discovered. Based on these discoveries, and comparative analyses of the structure of organisms (a field known as cladistics), it is possible to propose plausible "family trees" (phylogenies) connecting different types of organisms - modern molecular genetics methods, particularly genome (DNA) sequencing, have confirmed these predictions, and produced strong experimental support for the current view that all organisms currently living on the earth are part of the same family, that is they share a common ancestor, an ancestor that lived billions of years ago. The theory of evolution also predicts the older the rocks, the more different will the fossilized organisms found be from modern organisms. In rocks dated to be 410 million years old, we find fossils of various types of fish, but not fish that exist today; we do not find evidence of humans, there are, in fact, no mammals, no reptiles, no insects, and no birds. A second foundational premise of science is that all theories are restricted to natural phenomena, that is phenomena that can be observed and measured, either directly or indirectly. Explanations that invoke the supernatural, or the totally subjective, are by definition not scientific, since there is no imaginable experiment that could be done that might provide evidence one way or another for their validity. In an important sense, it does not matter whether these supernatural explanations are true (in the deepest sense) or not, they remain unscientific. Imagine an instrument that could detect the presence of angels – if such an instrument could be built, angels could be studied scientifically; their numbers and movements could be tracked and their structure and behaviors analyzed, it might even be possible to predict or control their behavior - they would cease to be supernatural and would become just another part of the natural world. Given these admitted arbitrary limitations on science as a discipline and an enterprise, it is rather surprising how well science works in explaining the world around us. At the same time, science has essentially nothing to say about the meaning of the world around us - although it is often difficult not to speculate on meaning based on current scientific theories. Given that all theories are tentative, and may be revised or abandoned, perhaps it is wise not to use scientific ideas to decide what is good or bad, right or wrong (morally). As we will see the history of atomic theory is rife with examples of one theory being found to be inadequate, upon which it is revised, extended and occasionally totally replaced by a newer theory that provide testable explanations for both old and new experimental evidence. This does not mean that the original theory was completely false – but rather that it was unable to fully capture the observable universe or to accurately predict newer observations. Older theories are generally subsumed as newer ones emerge - in fact, the newer theory must explain the failings of the older one. |
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Atoms: Invisible and Indivisible - some history: The ancient Greeks developed complex ideas about the nature of the universe (and the matter from which it was composed) that were accepted for a long time. However, in response to more careful observation and experimental analysis, these ideas were eventually superseded by more rigorous theories. In large part this involved a process by which people took old ideas seriously, and tried to explain and manipulate the world based on them. When their observations and manipulations failed to produce the expected (or desired) outcomes, such as turning base metals into gold, curing diseases or evading death altogether, they were more or less forced to revise their ideas, often abandoning older ideas for ideas that "worked". The development of atomic theories is intertwined with ideas about the fundamental nature of matter, not to mention the origin of the universe and its evolution. Most of the Greek Philosophers thought that matter was composed of some set of basic "elements", for example, the familiar Earth, Air, Fire, and Water. Some philosophers proposed the presence of a fifth element, known as quintessence or “aether”. These clearly inadequate ideas remain today as part of astrology and the signs of the Zodiac – a not particularly fitting tribute to some very serious thinkers. The original elements (that is Earth, Air, Fire and Water) were thought to be composed of tiny indestructible particles – called atoms by Leucippus and Democritus (who lived around 460 BCE)[optional link]. The atoms of different elements where assumed to be of different sizes and shapes, and their shapes directly gave rise to the properties of the particular element. For example the atoms of earth were thought to be cubic; their close packing made “earth” difficult to move and solid. The idea that the structure of atoms determines the observable properties of the material is one that we will return to, in a somewhat different form, time and again, and while the particulars were not correct, the basic idea turns out to be sound. |
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All in all the combined notions of the Greek philosophers provided a self-consistent and satisfactory basis for an explanation of the behavior of matter, as far as they could tell - or better put, all that they needed to know for their day to day purposes. The trap here is one that is very easy to fall into. That is: a satisfying explanation for a phenomenon does not necessarily mean that it is true. An explanation, even if it seems to be self-consistent and useful or comforting, is not scientific unless it makes testable quantitative predictions. For example: it was thought that different materials were made up of different proportions of the four ancient elements. Bones were made of water, earth and fire in the proportions 1:1:2, whereas flesh was composed of these elements in a ratio of 2:1:1.[from A History of Greek philosophy By William Keith Chambers Guthrie. p212.] Some philosophers even thought that the soul was composed of atoms or that atoms themselves had a form of consciousness, two ideas that seem quite foreign to (most of) us today. While these ideas are now considered preposterous (if not just silly), they contain a foreshadowing of the Law of Constant Proportions (which would come some 2300 years later and which we will deal with later in this chapter). Such ideas about atoms and elements provided logical and rational (non-supernatural) explanations for many of the properties of matter. But Greeks weren’t the only ancient people to come up with explanations for the nature of matter and its behavior. In fact it is thought that the root of the words alchemy and chemistry is the ancient Greek word Khem, their name for Egypt, where alchemy/chemistry are thought to have originated.[optional link] Similar theories were being developed in India at about the same time, although it is the Greek ideas about atoms that were preserved and used by the people who eventually developed our modern atomic theories. With the passage of time, ancient ideas about atoms and matter were kept alive by historians and chroniclers, in particular scholars in the Arabic world. During the European "Dark Ages" and into Medieval times, there were a few scattered revivals of ideas about atoms, but it was not until the Renaissance that the cultural and intellectual climate once again allowed the relatively free flowering of ideas. This included speculation on the nature of matter and atoms. Experimental studies based upon these ideas led to their revision and the eventual appearance of science as we now know it. It is also worth remembering that this relative explosion of new ideas was occasionally and sometimes vigorously opposed by religious institutions, leading to torture, confinement, and executions [Think Giordano Bruno and Galileo]. Identifying (and isolating) elements |
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Evidence for Atoms: The first scientific theory of atomic structure was proposed by John Dalton (1766 - 1844), a self taught Quaker [religious dissenters, that is non-Anglicans, were not allowed access to English universities at that time. ] living in Manchester, England38. In 1805 Dalton published his atomic theory to explain the observed law of multiple proportions. Rather surprisingly, Dalton never really explained what led him to propose his atomic theory, although he certainly used it to explain existing rules about how different elements combine. Among these rules (or Laws) was the observation that the total matter present in a system did not change when a chemical reaction occurred, although a reaction might lead to a change from a solid to a gas or vice versa. Inspection of his laboratory notebooks suggests that he first began to develop this atomic theory as he was experimenting on the nature of different gases and their solubility in water. In 1803 he wrote: This was the first indication that he was thinking about gases in terms of particles (atoms/molecules, that is combinations of atoms). In case you missed this extraordinary deduction (and it is very easy to do), Dalton made the leap to the idea of atoms with different weights from his observations that different gases dissolved in water in different amounts and the law of multiple proportions. Dalton’s atomic theory (1805) had a number of important points:
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The law of multiple proportions The law of multiple proportions is an empirical law, that is a law based on observation rather than theoretical logic. It states that when two elements (for example carbon and oxygen) combine to form more than one type of compound, such as carbon monoxide and carbon dioxide, the ratio of the mass of oxygen in carbon monoxide is always in some whole number to the mass of oxygen in carbon dioxide. Connecting the real world and the molecular world One problem chemists have is that we deal with things that happen at a scale that we cannot see (and is very difficult to imagine). As a result we have to develop a number of skills and tools to connect the molecular world with the world we can see. For example: a large part of the later sections of the book is taken up with developing ways to help you visualize molecular level structures and events. But, while thinking about the molecular level is important, it is also necessary to be able to connect those molecular changes with what we can see and measure in the world we live in. For example we might visualize a chemical reaction as a molecule of one reactant interacting with another molecule to give a product. We generally write reactions down in the form of equations, for example:
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| All the other elements have masses that are defined relative to this mass. So for example, the equation above could mean all these things: | ![]() |
A note on the conservation of matter: |
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The Divisible Atom Dalton’s theory of atoms as indivisible, indestructible, objects, of different sizes, weights, and perhaps shapes, depending on the element, held up for almost 100 years, although there was considerable dissent about whether atoms really existed, particularly among philosophers (a wacky bunch, if ever there was one). By 1900 the atomic theory was almost universally accepted by chemists. More evidence began to accumulate, more elements were discovered, and it even became possible to calculate the number of atoms in a particular sample. The first step along this direction was made by Amedeo Avogadro (1776 - 1856); in 1811 he proposed that, under conditions of equal temperature and pressure, equal volumes of gases contained equal numbers of particles (molecules) and that the densities of the gases (that is their weight divided by their volume) were proportional to the weight of the individual molecules. This was expanded upon by the Austrian high school teacher Josef Loschmidt (1821-1895) who, in 1865, combined Avogadro's conclusion with the assumption that atoms and molecules move very much as inelastic objects (think billiard balls). This enabled him to calculate the force a molecule would exert when traveling at a particular speed (something difficult to measure) and relate that to the pressure (something that can actually be measured). In fact, this assumption enabled physicists to deduce that the temperature of a gas is related to the average kinetic energy of the molecules within it - a concept we will return to shortly. Probing the substructure of atoms: The excitement about electricity and its possible uses prompted Alessandro Volta (1745 –1827) to develop the first battery, now known as a Voltaic Pile. He alternated sheets of two different metals, such as zinc and copper, with discs soaked in salt water (brine). It produced the first steady electrical current that, when applied to frog muscles caused them to contract. Such observations indicated that bioelectricity could be generated non-biologically, that it was no different than any other form of electricity. What neither Volta nor Galvani knew was the nature of electricity - what was it, exactly, and how did it "flow" from place to place? What was in the spark that jumped from finger to metal door knob, or from Benjamin Franklin's (1705 – 1790) kite string to his finger? What was this electrical “fluid” made of? |
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| Progress in the understanding of the nature and behavior of electricity continued throughout the 19th century, and the power of electricity was harnessed to produce dramatic changes in the way people lived and worked - powering factories, lighting houses and streets, etc. Yet there was no real deep of understanding as to the physical nature of electricity. It was known that electric charge came in two forms, positive and negative and that these charges were conserved, that is, they could not be created or destroyed (ideas first proposed by Franklin). The electrical (charged) nature of matter was well established, but not where that charge came from or ”what it was”. |
| A key step that began to unravel the idea of an indivisible atom was made by J. J. Thompson (1856 – 1940), another Mancunian40. While the idea of electricity, was now well appreciated, Thompson and other scientists wanted to study it in a more controlled manner. They used what were (and are now) known as cathode ray tubes (CRTs); once common in televisions, these are being replaced by various “flat screen” devices. | ![]() |
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In all of these experiments, it needs to be stressed that "positive" and "negative" are meant to indicate opposite, and are assigned by convention - that means that we could decide tomorrow that positive was negative, and negative positive, and nothing would change (as long as we were consistent). From these experiments, Thompson concluded that the cathode rays were carried by charged discrete particles (he called them corpuscles) and he assigned these particles a "negative" charge. But the truly stunning conclusion that he reached was that these particles must come from within the atoms of the metal cathode. Since the type of metal did not affect the nature or behavior of the cathode rays, he assumed that these particles were not newly created, but must pre-exist within the atoms of the cathode and moreover, that identical particles were present in all atoms – not just the atoms of one particular metal. Do you see how he jumps from experimental results using a few metals to all elements, all atoms? Of course, we now know these particles as electrons, but it is difficult to imagine what a huge impact this new theory had on scientists at the time. “Since electrons can be produced by all chemical elements, we must conclude that they enter the constitution of all atoms. We have thus taken our first step in understanding the structure of the atom” – J. J. Thompson. The Atomic Theory, Oxford, Clarendon Press. 1914.[link] The discovery of the electron made the old idea of an atom as a little indestructible billiard ball-like object obsolete, and necessitated a new model. It is an example of a paradigm shift [A term made popular (although often misunderstood) by T. S. Kuhn, The Structure of Scientific Revolutions, 1st. ed., Chicago: Univ. of Chicago Pr., 1962]– a fundamental change in scientific thinking driven by new evidence. Thompson’s first version of this new model became known as the “plum pudding” model 44. His basic idea was that the atom is a ball of positively charged, but apparently amorphous matter with electrons studded here and there (like the raisins in the pudding); since it contained equal numbers of positive and negative charges the overall structure was electrically neutral. Subsequent work by Thompson and Robert A. Millikan (1868 – 1953) established that all electrons are identical, each with the same (very small) mass and negative charge. The mass of an electron is less than 1000th of the mass of a hydrogen atom. Thompson's proposed plum pudding model of the atom spurred much experimental and theoretical work and led to a remarkable number of subsequent discoveries. For example, it was soon recognized that the β (beta) particles emitted by some radioactive minerals and elements, were, in fact, electrons. Other studies found that the number of electrons present in the atoms of a particular element was roughly proportional to half the element's atomic weight, although why this should be the case was unclear. Based on these experimental results Rutherford reasoned that the positively charged α particles were being repelled by positive parts of the atom. Since only a very small percentage of α particles were deflected, only a very small region of each atom could be positively charged. That is: the positive charge in an atom could not be spread out more or less uniformly as the plum pudding model assumed, instead they must be concentrated in a very small region. This implied that most of the atom is empty (remember the “void” of the ancient Greeks?) or occupied by something that posed little or no resistance to the passage of the α particles. Again we see a scientist making a huge intuitive leap from the experimental evidence to a hypothesis that is consistent with that evidence and that makes specific predictions that can be confirmed or falsified by further experiment and observation. Rutherford's model – which became known as the planetary model, postulated a very (very) small nucleus where all of the positive charge and nearly all of the mass of the atom was located, this nucleus was encircled by electrons. In 1920 Rutherford went on to identify the unit of positive charge and call it the proton; in 1932, James Chadwick (1891-1974)(who co-incidentally studied at the University of Manchester) identified a second component of the nucleus, the neutron. Neutrons are heavy, like protons - in fact they are slightly heavier than protons, but have no charge. Neutrons are not completely stable, however, and can decay into a proton, an electron, and another particle, called an anti-neutrino. Both the electron (a β-particle) and the anti-neutrino are expelled from the nucleus while the proton remains. Changing a neutron into a proton changes the identity of the element. |
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Interactions between atoms and molecules. Where the electrons actually are, however, is a trickier question to answer, because of quantum mechanical considerations, specifically the Heisenberg uncertainty principal (which we will return to in the next chapter). For now let’s just assume the electrons are outside the nucleus and moving. We can think of them as if they were a cloud of electron density – rather than particles whizzing around. This simple model captures important features that enables us to begin to consider how atoms interact with one another to form molecules and how those molecules can be rearranged – real chemistry! One thing we can ignore (for now) are the interactions involved in holding the nucleus together. There is an attractive force between neutrons and protons, known as the strong nuclear force, that holds these particles together in the nucleus. This is the strongest of all known forces in the universe, approximately 137 times stronger than the electrostatic force, but it acts only at very short ranges, approximately 10-15 m, or about the diameter of the nucleus. The other force involved in nuclear behavior, the "weak force", plays a role in nuclear stability, specifically the stability of neutrons, but it has an even shorter range of action (10-18 m). Since the nucleus is much smaller than the atom itself, we can (and will) ignore the weak and strong forces when we consider chemical interactions. The only other force that appears to exist in the universe is gravity, but it is so weak (more than 10-37 times weaker than the electrostatic force), that we can ignore it from the perspective of chemistry (although it does have relevance for the biology of dinosaurs, elephants, whales, and astronauts). One obvious feature of the world that we experience is that it is full of solid things, things that get in each other's way. Moreover, there is a relationship between temperature and the form things take - consider water. At various temperatures water can be a solid (ice), a liquid, or a gas (water vapor). More unfamiliar substances, such as helium, carbon dioxide, methane, and propane display similar behaviors, changing from a gas to a liquid or solid as the temperature drops. Understanding why, and under what conditions these transitions occur, and why different substances change their "phase" under different conditions will lead us to a clearer understanding of how atoms and molecules interact with one another. If atoms and molecules did not interact with one another, one might expect to be able to walk through walls (since atoms are mostly empty space), but clearly this is not the case. Similarly, you would not “hold together” if your atoms, and the molecules they form, failed to interact. As we will see all atoms and molecules attract one another; a fact that follows directly from what we know about the structure of atoms (and molecules). |
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Interactions between atoms – a range of effects: Our model of the interactions between atoms will involve (initially) only electrostatic interactions - that is interactions between electrically charged particles, electrons and protons. Let us consider how atoms interact with one another. Taken as a whole, atoms are electrically neutral, but they are composed of electrically charged particles. Moreover, their electrons behave as moving objects [Yes we did tell you to think of electrons as a cloud - because this is a helpful model - but electrons are particles, in fact they appear to be quite close to perfect spheres in shape, In fact “The experiment, which spanned more than a decade, suggests that the electron differs from being perfectly round by less than 0.000000000000000000000000001 cm. This means that if the electron was magnified to the size of the solar system, it would still appear spherical to within the width of a human hair. (Hudson et al "Improved measurement of the shape of the electron" DOI: 10.1038/nature10104).]. While the probability of finding an electron is spread uniformly around an atom when averaged over time; at any one instant there is a probability that the electrons are more on one side of the atom than the other. This leads to momentary fluctuations in the charge density around the atom and leads to a slight charge build up, with one side of the atom being slightly positive and one side being slightly negative. This produces what is known as an instantaneous and transient electrical dipole - a separation of charge. As one atomic dipole nears another atom it will affect the electron density distribution, so for example if the slightly positive end of the atom is located next to another atom, it will attract the electron(s) in the other atom. This results in an overall attraction between the atoms that varies as 1/r6 (Note that this is different than the attraction between fully charged species - the Coulombic attraction -which varies as 1/r2) ?What does that mean in practical terms? Well, most importantly it means that the effects of the interaction will be felt only when the two atoms are quite close to one another. |
| As two atoms approach, they will be increasingly attracted to one another. This attraction has its limit, however - when the atoms get close enough the repulsive effects between the negatively charged electrons and the positively charged nuclei increases very rapidly (look back at the opening quote from Feynman). | ![]() |
The repulsive interactions between nuclei are easier to imagine, since they behave more like billiard balls rather than clouds, but bear in mind that the electron clouds also repel each other if they get too close. Reflect back to Rutherford's experiment (please!) He accelerated positively charged α particles, toward a sheet of gold atoms. As an α particle approaches a gold atom's nucleus, the positively (+2) charged α particle and the gold atom’s positively (+79) nucleus begin to repel each other. If no other factors were involved the force of repulsion would approach infinity as the distance between the nuclei (r) approached 0 (you should be able to explain why.) But infinite forces are not something that happens in the real or the atomic/subatomic world, if only because the total energy in the universe is not infinite. As the distance between the α particle and gold nucleus approaches zero, the repulsive interaction grows strong enough to slow the incoming α particle and then push it away from the target particle. If the target particle is heavy compared to the incoming particle, as it was in Rutherford's experiments, the target (gold atoms - which weigh about 50 times as much as the α particle) will not move much, while the incoming α particle will be reflected away. But, f the target and incoming particle are of similar mass, then both will be affected by the interaction and both will move. Interestingly, if the incoming particle had enough initial energy to get close enough (within about 10-15 m) to the target nucleus, then the strong nuclear force of attraction would come into play and start to stabilize the system. The result would be the fusion of the two nuclei, and the creation of a different element, a process that occurs only in very high energy systems such as the center of stars or during a stellar explosion (a supernova). We will return to this idea in chapter 3. Interacting atoms: energy conservation and conversion: As two atoms/molecules approach each other they will feel the force of attraction caused by the electron density distortions, these are known as London dispersion forces (which we will abbreviate as LDF). The effects of these LDF’s depends upon their strength and on the atoms/molecules’ kinetic energies. The type of attraction between atoms and molecules that involves LDF is known as a van der Waals interaction (there are various types of van der Waals interactions which we will get to later). To simplify things (as physicists are wont to do), let us consider a very specific situation. If we assume that there are two isolated atoms, atom1 and atom2; the atoms are at rest with respect to one another, but close enough so that the LDFs between them are significant. For this to occur they have to be quite close, because LDFs, which result from the movement of electrons, fall off as 1/r6 where r is the distance between the two atoms. In response to the attractive LDF’s, the atoms begin to move toward each other – potential energy associated with the atoms initial state is converted into kinetic energy (EK = ½mv2). If there was no attraction, the potential energy of the system would be zero. |
| As the atoms begin to slow down, their kinetic energy is converted back into potential energy. They will eventually stop and then be repelled from one another - potential energy will be converted back into kinetic energy. As they move away, however, repulsion will be replaced by attraction, and they will slow - their kinetic energy will be converted back into potential energy. With no other factors acting within the system, the two atoms will oscillate forever. |
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Here we have a core principle that we will return to time and again - a stabilizing interaction always lowers the potential energy of the system, and conversely, a destabilizing interaction always raises the energy of the system. In an isolated system with only two atoms, this oscillation would continue forever because there is no way to change the energy of the system. This situation doesn’t occur in “real life” because two-atom systems do not occur. For example even in a gas, where the atoms are far apart, there are typically large numbers of atoms that have a range of speeds (and kinetic energies), present in a system . These atoms frequently collide and transfer energy. Therefore, when two atoms collide and start to oscillate, some of the energy may be transferred to other particles by collisions. If this happens a stable interaction can form between the two particles and make them stick together. If more particles approach, they can also become attracted, and if their extra energy is transferred by collisions, the particles can form a bigger and bigger “clump”. As we discussed earlier, London dispersion forces arise due to the fluctuations of electron density around nuclei, and are a feature common to all atoms; all atoms/molecules attract one another in this manner. The distance between atoms/molecules where this attraction is greatest is known as the van der Waals radius of the atom/molecule – if atoms/molecules move closer to one another than their van der Waals radii, they repel one another. The van der Waals radius of an atom is characteristic for each type of atom/element. As mentioned earlier, it is only under conditions of extreme temperature and pressure that the nuclei of the two atoms can fuse together to form a new type of atom; such a nuclear/atomic fusion event results in the interconversion of matter into energy. Interactions between helium atoms and hydrogen molecules: When two atoms of helium approach each other LDFs come into play and a van der Waals interaction develops. In the case of He, the interaction potential energy drop is quite small (that is: the stabilization due to the interaction) and it does not take much energy to knock the two atoms apart. This energy is supplied by collisions with other He atoms. Helium melts at ~1K (−272.2 ºC) and boils at ~4K (−268.93ºC), only a few degrees above absolute zero 0K (−273.15 ºC). Meaning that at all temperatures above ~4K, there is enough kinetic energy in the atoms of the system to disrupt the van der Waals interactions between He atoms. The lack of stable interaction at these “higher” temperatures means that helium atoms do not stick together above 4K; helium is a gas at temperatures above 4K. Now let us contrast the behavior of helium with that of hydrogen (H). As two hydrogen atoms approach one another, they form a much more stable interaction (about 1000 times stronger than the He-He van der Waals interactions. In an H-H interaction, the atoms are held together by the attraction of each nucleus for both electrons. This leads to a potential energy minimum for the two interacting hydrogen atoms that is much deeper than that for He-He. Because of its radically different stability, the H-H system gets a new name, it is known as molecular hydrogen or H2, and the interaction between the H atoms is known as a covalent bond. In order to separate the hydrogen molecule back into two atoms, that is, to break the covalent bond between them, we have to supply energy. 51 This energy can take several forms: energy delivered by molecular collisions with surrounding molecules or electromagnetic energy due to the absorption of light ?are some of the ways covalent bonds can be broken, and we will return to them later. |
| To break a H-H covalent bond, you will need to heat the system to around 5000K. On the other hand, to break the van der Waals interactions between H2 molecules, the system temperature only needs to rise to ~20K, above this temperature H2 is a gas; the interactions between individual H2 molecules are not strong enough to resist the kinetic energy of colliding molecules. Now you may ask yourself, why does H2 boil at a higher temperature than He? Good question! The answer is addressed by the web activity on interactions. It turns out that the strengths of these types of interactions depend upon several factors, including shape of the molecule, surface area, and number of electrons. For example, the greater the surface areas shared between interacting atoms or molecules the greater the London dispersion forces experienced and the stronger the resulting van der Waals interaction. Another factors is the ability of the electron cloud to become charged, a property known as polarizability. Polarizability is related to the “floppiness” of the electron cloud, and as a rough guide, the further away from the nucleus the electrons are - the more polarizable (moveable or floppy) the electron cloud becomes. We will return to this and related topics later on. As we will see, larger molecules with more complex geometries, such as biological macromolecules - proteins and nucleic acids – can interact through more surface area and polarizable regions, leading to correspondingly stronger van der Waals interactions. |
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At this point, you are probably (or should be) asking yourself some serious questions, such as, why don’t helium atoms form covalent bonds with one another? Why does a hydrogen atom form only one covalent bond? What happens when other kinds of atoms interact? To understand the answers to these questions, we need to consider how the structure of atoms differs between the different elements, which is the subject of the next chapter. |
| 12-Apr-2012 |