#set document(title: "11.1 Introduction to Particle Physics", author: "OpenStax / XYZ Homework") #set page(width: 8.5in, height: auto, margin: 1in) #import "@preview/cetz:0.5.2" #set text(font: ("STIX Two Text", "Libertinus Serif", "New Computer Modern"), size: 10.5pt, lang: "en") #show math.equation: set text(font: ("STIX Two Math", "New Computer Modern Math")) #set par(justify: true, leading: 0.62em, spacing: 0.9em) #set enum(spacing: 1.1em) // room between list items so tall inline fractions don't collide #set list(spacing: 1.1em) #set table(stroke: 0.5pt + rgb("#c7ccd3")) #let BLUE = rgb("#183B6F") // brand navy — section bars + example/solution labels (white on navy 11.09:1) #let ORANGE = rgb("#A94509") // brand primary-700 — AA-safe deep orange for TEXT (5.93:1 on white; raw brand #F37021 is 2.94:1 and must never carry text) #let RED = rgb("#DC2626") // brand error-600 #let GREEN = rgb("#059669") // brand success-600 (decoration only; small green text uses green-text #007942) #show heading.where(level: 1): it => block(width: 100%, above: 0pt, below: 16pt, fill: gradient.linear(BLUE, rgb("#2C5AA0")), inset: (x: 14pt, y: 12pt), radius: 3pt, text(fill: white, weight: "bold", size: 19pt, it.body)) #show heading.where(level: 2): it => block(width: 100%, above: 18pt, below: 10pt, fill: BLUE, inset: (x: 10pt, y: 6pt), radius: 2pt, text(fill: white, weight: "bold", size: 12pt, it.body)) #show heading.where(level: 3): it => text(fill: ORANGE, weight: "bold", size: 12.5pt, it.body) #show heading.where(level: 4): it => text(fill: BLUE, weight: "bold", size: 10.5pt, it.body) #let examplebox(label, title, body) = block(width: 100%, breakable: true, fill: rgb("#EFF1F5"), stroke: 0.5pt + rgb("#CFDDF0"), radius: 4pt, inset: 10pt, above: 12pt, below: 12pt)[ #block(below: 6pt)[#box(fill: BLUE, inset: (x: 6pt, y: 2pt), radius: 2pt, text(fill: white, weight: "bold", size: 8.5pt, label)) #h(0.4em) #strong[#title]] #body] // rail = decorative left rule (raw brand token); labelcolor = AA-safe label text shade #let notebox(label, rail, labelcolor, tint, body) = block(width: 100%, breakable: true, fill: tint, stroke: (left: 3pt + rail), inset: (left: 10pt, rest: 8pt), radius: (right: 4pt), above: 11pt, below: 11pt)[ #text(fill: labelcolor, weight: "bold", size: 7.5pt, tracking: 0.5pt)[#upper(label)] #linebreak() #body] #let solutionbox(body) = block(above: 4pt, below: 8pt)[ #text(fill: BLUE, weight: "bold", size: 8.5pt)[Solution] #linebreak() #body] #let figph(msg) = block(width: 100%, height: 60pt, fill: rgb("#f6f7f9"), stroke: (paint: rgb("#c7ccd3"), dash: "dashed"), radius: 4pt, inset: 10pt)[ #align(center + horizon, text(fill: rgb("#889"), style: "italic", size: 9pt, msg))] // Standardize inlined figure sizes: measure the natural CeTZ canvas, then scale to a // consistent envelope (aspect-aware; see build_typst.py FIG_* constants). Unlike the // print preamble, dimensions are FLOORED: in an editor a user can trim a figure to a // degenerate 1-D shape (a bare line), and w/h or tw/w would then divide by zero. #let _STD_W = 3.5 #let _WIDE_W = 5.6 #let _MAX_H = 3.4 #let _ASPECT_WIDE = 2.2 #let _UPSCALE_MAX = 1.15 #let stdfig(body) = context { let m = measure(body) let w = calc.max(m.width / 1in, 0.01) let h = calc.max(m.height / 1in, 0.01) let tw = if w / h > _ASPECT_WIDE { _WIDE_W } else { _STD_W } let s = calc.min(tw / w, _MAX_H / h, _UPSCALE_MAX) align(center, box(scale(x: s * 100%, y: s * 100%, reflow: true, body))) } #show figure: set block(breakable: false) #set figure(gap: 8pt) #show figure.caption: set text(size: 8.5pt, fill: rgb("#555")) == 11.1#h(0.6em)Introduction to Particle Physics Elementary particle physics is the study of fundamental particles and their interactions in nature. Those who study elementary particle physics—the particle physicists—differ from other physicists in the scale of the systems that they study. A particle physicist is not content to study the microscopic world of cells, molecules, atoms, or even atomic nuclei. They are interested in physical processes that occur at scales even smaller than atomic nuclei. At the same time, they engage the most profound mysteries in nature: How did the universe begin? What explains the pattern of masses in the universe? Why is there more matter than antimatter in the universe? Why are energy and momentum conserved? How will the universe evolve? The field of particle physics was developed through observations that could not be initially explained, but which led researchers to deepen their investigations and develop conclusions led to an entire sub-discipline of physics, with substantial applications across science and industry. The discovery of elementary particles was due in part to the development and often ingenuous application of new technologies. As discussed earlier, Ernest Rutherford's experiments using photographic plates were, essentially, the initial forays into particle physics. Austrian physicist Marietta Blau began advancing the photographic plate process, known as nuclear emulsion, through the incorporation of new materials and the creation of new techniques to run experiments. She was able to detect proton tracks and determine the energy of neutrons and protons. By placing specially prepared plates on the top of a mountain to capture cosmic rays, she recorded the first evidence of nuclear disintegration. Debendra Mohan Bose, Bibha Chowdury, Cecil Powell, and others built on this knowledge and discovered new particles such as the meson. These efforts would lead to an increasingly deeper knowledge of the smallest particles of matter, their applications, and the forces within atoms. === Four Fundamental Forces An important step to answering these questions is to understand particles and their interactions. Particle interactions are expressed in terms of four #strong[fundamental force]#strong[s]. In order of decreasing strength, these forces are the #strong[strong nuclear force], the electromagnetic force, the #strong[weak nuclear force], and the gravitational force. + #strong[Strong nuclear force.] The strong nuclear force is a very strong attractive force that acts only over very short distances (about #math.equation(block: false, alt: "10 to the power −15 m")[$10^(−15) #h(0.2em) "m"$]). The strong nuclear force is responsible for binding protons and neutrons together in atomic nuclei. Not all particles participate in the strong nuclear force; for instance, electrons and neutrinos are not affected by it. As the name suggests, this force is much stronger than the other forces. + #strong[Electromagnetic force.] The electromagnetic force can act over very large distances (it has an infinite range) but is only 1/100 the strength of the strong nuclear force. Particles that interact through this force are said to have “charge.” In the classical theory of static electricity (Coulomb’s law), the electric force varies as the product of the charges of the interacting particles, and as the inverse square of the distances between them. In contrast to the strong force, the electromagnetic force can be attractive or repulsive (opposite charges attract and like charges repel). The magnetic force depends in a more complicated way on the charges and their motions. The unification of the electric and magnetic force into a single electromagnetic force (an achievement of James Clerk Maxwell) stands as one of the greatest intellectual achievements of the nineteenth century. This force is central to scientific models of atomic structure and molecular bonding. + #strong[Weak nuclear force.] The weak nuclear force acts over very short distances #math.equation(block: false, alt: "open parenthesis 10 to the power −15 m close parenthesis")[$( 10^(−15) #h(0.2em) "m" )$] and, as its name suggest, is very weak. It is roughly #math.equation(block: false, alt: "10 to the power −6")[$10^(−6)$] the strength of the strong nuclear force. This force is manifested most notably in decays of elementary particles and neutrino interactions. For example, the neutron can decay to a proton, electron, and electron neutrino through the weak force. The weak force is vitally important because it is essential for understanding stellar nucleosynthesis—the process that creates new atomic nuclei in the cores of stars. + #strong[Gravitational force.] Like the electromagnetic force, the gravitational force can act over infinitely large distances; however, it is only #math.equation(block: false, alt: "10 to the power −38")[$10^(−38)$] as strong as the strong nuclear force. In Newton’s classical theory of gravity, the force of gravity varies as the product of the masses of the interacting particles and as the inverse square of the distance between them. This force is an attractive force that acts between all particles with mass. In modern theories of gravity, this force behavior is considered a special case for low-energy macroscopic interactions. Compared with the other forces of nature, gravity is by far the weakest. The fundamental forces may not be truly “fundamental” but may actually be different aspects of the same force. Just as the electric and magnetic forces were unified into an electromagnetic force, physicists in the 1970s unified the electromagnetic force with the weak nuclear force into an #strong[electroweak force]. Any scientific theory that attempts to unify the electroweak force and strong nuclear force is called a #strong[grand unified theory], and any theory that attempts to unify all four forces is called a #strong[theory of everything]. We will return to the concept of unification later in this chapter. === Classifications of Elementary Particles A large number of subatomic particles exist in nature. These particles can be classified in two ways: the property of spin and participation in the four fundamental forces. Recall that the spin of a particle is analogous to the rotation of a macroscopic object about its own axis. These types of classification are described separately below. ==== Classification by spin Particles of matter can be divided into #strong[fermion]#strong[s] and #strong[boson]#strong[s]. Fermions have half-integral spin #math.equation(block: false, alt: "open parenthesis the fraction 1 over 2 ℏ , the fraction 3 over 2 ℏ , … close parenthesis")[$( frac(1, 2) ℏ , #h(0.2em) frac(3, 2) ℏ , #h(0.2em) "…" )$] and bosons have integral spin #math.equation(block: false, alt: "open parenthesis 0 ℏ , 1 ℏ , 2 ℏ , … close parenthesis .")[$( 0 ℏ , #h(0.2em) 1 ℏ , 2 ℏ , "…" ) .$] Familiar examples of fermions are electrons, protons, and neutrons. A familiar example of a boson is a photon. Fermions and bosons behave very differently in groups. For example, when electrons are confined to a small region of space, #strong[Pauli’s exclusion principle] states that no two electrons can occupy the same quantum-mechanical state. However, when photons are confined to a small region of space, there is no such limitation. The behavior of fermions and bosons in groups can be understood in terms of the property of indistinguishability. Particles are said to be “indistinguishable” if they are identical to one another. For example, electrons are indistinguishable because every electron in the universe has exactly the same mass and spin as all other electrons—“when you’ve seen one electron, you’ve seen them all.” If you switch two indistinguishable particles in the same small region of space, the square of the wave function that describes this system and can be measured #math.equation(block: false, alt: "open parenthesis | ψ | squared close parenthesis")[$( | ψ |^(2) )$] is unchanged. If this were not the case, we could tell whether or not the particles had been switched and the particle would not be truly indistinguishable. Fermions and bosons differ by whether the sign of the wave function (#math.equation(block: false, alt: "ψ")[$ψ$])— not directly observable—flips: #math.equation(block: true, alt: "ψ → − ψ (indistinguishable fermions),; ψ → plus ψ (indistinguishable bosons).")[$ψ → "−" ψ #h(0.2em) "(indistinguishable fermions)," \ ψ → + ψ #h(0.2em) "(indistinguishable bosons)."$] Fermions are said to be “antisymmetric on exchange” and bosons are “symmetric on exchange.” Pauli’s exclusion principle is a consequence of #strong[exchange symmetry] of fermions—a connection developed in a more advanced course in modern physics. The electronic structure of atoms is predicated on Pauli’s exclusion principle and is therefore directly related to the indistinguishability of electrons. ==== Classification by force interactions Fermions can be further divided into #strong[quark]#strong[s] and #strong[lepton]#strong[s]. The primary difference between these two types of particles is that quarks interact via the strong force and leptons do not. Quarks and leptons (as well as bosons to be discussed later) are organized in . The upper two rows (first three columns in purple) contain six quarks. These quarks are arranged into two particle families: up, charm, and top (#emph[u], #emph[c], #emph[t]), and down, strange, and bottom (#emph[d], #emph[s], #emph[b]). Members of the same particle family share the same properties but differ in mass (given in #math.equation(block: false, alt: "MeV/ c squared")[$"MeV/" c^(2)$]). For example, the mass of the top quark is much greater than the charm quark, and the mass of the charm quark is much greater than the up quark. All quarks interact with one another through the strong nuclear force. #figure(figph[This is a table with four rows and four columns. The first three cells in the first and second rows are labeled quarks. The first three cells in the third and fourth rows are labeled leptons. The last column is labeled bosons, forces. Each cell has the name of a particle, it’s symbol, mass, charge, and spin. In the first row, these values, in that order, are: cell one: up, u, 2.4 MeV, 2 by 3, 1 by 2; cell two: charm, c, 1.27 GeV, 2 by 3, 1 by 2; cell three, top, t, 171.2 GeV, 2 by 3, 1 by 2; cell four: photon, gamma, 0, 0, 1. In row two, these values, in that order, are: cell one: down, d, 4.8 MeV, minus 1 by 3, 1 by 2; cell two: strange, s, 104 MeV, minus 1 by 3, 1 by 2; cell three: bottom, b, 4.2 GeV, minus 1 by 3, 1 by 2; cell four: gluon, 0, 0, 1. In row three, these values, in that order, are: cell one: electron neutrino, v subscript e, less than 2.2 eV, 0, 1 by 2; cell two: muon neutrino, v subscript mu, less than 0.17 MeV, 0, 1 by 2; cell three: tau neutrino, v subscript tau, less than 15.5 MeV, 0, 1 by 2; cell four: weak force, z raised to 0, 91.2 GeV, 0,1. In row four, these values, in that order, are: cell one: electron, e, 0.511 MeV, minus 1, 1 by 2; cell two: muon, mu, 105.7 MeV, minus 1, 1 by 2; cell three: tau, tau, 1.777 GeV, minus 1, 1 by 2; weak force, w plus minus, 80.4 GeV, plus minus 1, 1.], alt: "This is a table with four rows and four columns. The first three cells in the first and second rows are labeled quarks. The first three cells in the third and fourth rows are labeled leptons. The last column is labeled bosons, forces. Each cell has the name of a particle, it’s symbol, mass, charge, and spin. In the first row, these values, in that order, are: cell one: up, u, 2.4 MeV, 2 by 3, 1 by 2; cell two: charm, c, 1.27 GeV, 2 by 3, 1 by 2; cell three, top, t, 171.2 GeV, 2 by 3, 1 by 2; cell four: photon, gamma, 0, 0, 1. In row two, these values, in that order, are: cell one: down, d, 4.8 MeV, minus 1 by 3, 1 by 2; cell two: strange, s, 104 MeV, minus 1 by 3, 1 by 2; cell three: bottom, b, 4.2 GeV, minus 1 by 3, 1 by 2; cell four: gluon, 0, 0, 1. In row three, these values, in that order, are: cell one: electron neutrino, v subscript e, less than 2.2 eV, 0, 1 by 2; cell two: muon neutrino, v subscript mu, less than 0.17 MeV, 0, 1 by 2; cell three: tau neutrino, v subscript tau, less than 15.5 MeV, 0, 1 by 2; cell four: weak force, z raised to 0, 91.2 GeV, 0,1. In row four, these values, in that order, are: cell one: electron, e, 0.511 MeV, minus 1, 1 by 2; cell two: muon, mu, 105.7 MeV, minus 1, 1 by 2; cell three: tau, tau, 1.777 GeV, minus 1, 1 by 2; weak force, w plus minus, 80.4 GeV, plus minus 1, 1.", caption: [The families of subatomic particles, categorized by the types of forces with which they interact.]) Ordinary matter consists of two types of quarks: the up quark (elementary charge, #math.equation(block: false, alt: "q equals plus 2 / 3")[$q = + 2 "/" 3$]) and the down quark #math.equation(block: false, alt: "open parenthesis q equals −1 / 3 close parenthesis .")[$( q = −1 "/" 3 ) .$] Heavier quarks are unstable and quickly decay to lighter ones via the weak force. Quarks bind together in groups of twos and threes called #strong[hadron]#strong[s] via the strong force. Hadrons that consist of two quarks are called #strong[mesons], and those that consist of three quarks are called #strong[baryons]. Examples of mesons include the pion and kaon, and examples of baryons include the familiar proton and neutron. A proton is two up quarks and a down quark #math.equation(block: false, alt: "open parenthesis p equals u u d , q equals +1 close parenthesis")[$( "p" = u u d , #h(0.2em) q = "+1" )$] and a neutron is one up quark and two down quarks (#math.equation(block: false, alt: "n equals u d d")[$"n" = u d d$], #math.equation(block: false, alt: "q equals 0")[$q = 0$]). Properties of sample mesons and baryons are given in . Quarks participate in all four fundamental forces: strong, weak, electromagnetic, and gravitational. The lower two rows in the figure (in green) contain six leptons arranged into two particle families: electron, muon, and tau (#math.equation(block: false, alt: "e , μ , τ")[$e , μ , τ$]), and electron neutrino, muon neutrino, and tau neutrino (#math.equation(block: false, alt: "υ sub e , υ sub μ , υ sub τ")[$υ_(e) , υ_(μ) , υ_(τ)$]). The muon is over 200 times heavier than an electron, but is otherwise similar to the electron. The tau is about 3500 times heavier than the electron, but is otherwise similar to the muon and electron. Once created, the muon and tau quickly decay to lighter particles via the weak force. Leptons do not participate in the strong force. Quarks and leptons will be discussed later in this chapter. Leptons participate in the weak, electromagnetic, and gravitational forces, but do not participate in the strong force. Bosons (shown in red) are the force carriers of the fermions. In this model, leptons and quarks interact with each other by sending and receiving bosons. For example, Coulombic interaction occurs when two positively charged particles send and receive (exchange) photons. The photons are said to “carry” the force between charged particles. Likewise, attraction between two quarks in an atomic nucleus occurs when two quarks send and receive #strong[gluon]#strong[s]. Additional examples include #strong[W and Z boson]#strong[s] (which carry weak nuclear force) and gravitons (which carry gravitational force). The Higgs boson is a special particle: When it interacts with other particles, it endows them not with force but with mass. In other words, the Higgs boson helps to explains #emph[why] particles have mass. These assertions are part of a tentative but very productive scientific model (the Standard Model) discussed later. === Particles and Antiparticles In the late 1920s, the special theory of relativity and quantum mechanics were combined into a relativistic quantum theory of the electron. A surprising result of this theory was the prediction of two energy states for each electron: One is associated with the electron, and the other is associated with another particle with the same mass of an electron but with a charge of #math.equation(block: false, alt: "e to the power plus")[$"e"^(+)$]. This particle is called the antielectron or #strong[positron]. The positron was discovered experimentally in the 1930s. Soon it was discovered that for every particle in nature, there is a corresponding #strong[antiparticle]. An antiparticle has the same mass and lifetime as its associated particle, and the opposite sign of electric charge. These particles are produced in high-energy reactions. Examples of high-energy particles include the antimuon (#math.equation(block: false, alt: "μ to the power plus")[$μ^(+)$]), anti-up quark (#math.equation(block: false, alt: "u −")[$limits(u)^("−")$]), and anti-down quark #math.equation(block: false, alt: "open parenthesis d − close parenthesis .")[$( limits(d)^("−") ) .$] (Note that antiparticles for quarks are designated with an over-bar.) Many mesons and baryons contain antiparticles. For example, the antiproton (#math.equation(block: false, alt: "p −")[$limits("p")^("−")$]) is #math.equation(block: false, alt: "u − u − d −")[$limits(u)^("−") limits(u)^("−") limits(d)^("−")$] and the positively charged pion #math.equation(block: false, alt: "open parenthesis π to the power plus close parenthesis")[$( π^(+) )$] is #math.equation(block: false, alt: "u d −")[$u limits(d)^("−")$]. Some neutral particles, such as the photon and the #math.equation(block: false, alt: "π to the power 0")[$π^(0)$] meson, are their own antiparticles. Sample particles, antiparticles, and their properties are listed in . #figure(table( columns: 6, align: left, inset: 6pt, [], [Particle name], [Symbol], [Antiparticle], [Mass #math.equation(block: false, alt: "open parenthesis MeV/ c squared close parenthesis")[$( "MeV/" c^(2) )$]], [Average lifetime (s)], [Leptons], [], [], [], [], [], [], [Electron], [#math.equation(block: false, alt: "e to the power −")[$"e"^("−")$]], [#math.equation(block: false, alt: "e to the power plus")[$"e"^(+)$]], [0.511], [Stable], [], [Electron neutrino], [#math.equation(block: false, alt: "υ sub e")[$υ_(e)$]], [#math.equation(block: false, alt: "υ sub e —")[$limits(υ_(e))^("—")$]], [#math.equation(block: false, alt: "approximately equals 0")[$≈ 0$]], [Stable], [], [Muon], [#math.equation(block: false, alt: "μ to the power −")[$μ^("−")$]], [#math.equation(block: false, alt: "μ to the power plus")[$μ^(+)$]], [105.7], [#math.equation(block: false, alt: "2.20 times 10 to the power −6")[$2.20 #h(0.2em) × #h(0.2em) 10^(−6)$]], [], [Muon neutrino], [#math.equation(block: false, alt: "υ sub μ")[$υ_(μ)$]], [#math.equation(block: false, alt: "υ sub μ —")[$limits(υ_(μ))^("—")$]], [#math.equation(block: false, alt: "approximately equals 0")[$≈ 0$]], [Stable], [], [Tau], [#math.equation(block: false, alt: "τ to the power −")[$τ^("−")$]], [#math.equation(block: false, alt: "τ to the power plus")[$τ^(+)$]], [1784], [#math.equation(block: false, alt: "less than 4 times 10 to the power −13")[$< 4 #h(0.2em) × #h(0.2em) 10^(−13)$]], [], [Tau neutrino], [#math.equation(block: false, alt: "υ sub τ")[$υ_(τ)$]], [#math.equation(block: false, alt: "υ sub τ —")[$limits(υ_(τ))^("—")$]], [#math.equation(block: false, alt: "approximately equals 0")[$≈ 0$]], [Stable], [Hadrons], [], [], [], [], [], [Baryons], [Proton], [p], [#math.equation(block: false, alt: "p −")[$limits("p")^("−")$]], [938.3], [Stable], [], [Neutron], [n], [#math.equation(block: false, alt: "n −")[$limits("n")^("−")$]], [939.6], [920], [], [Lambda], [#math.equation(block: false, alt: "Λ to the power 0")[$"Λ"^(0)$]], [#math.equation(block: false, alt: "Λ to the power 0 —")[$limits("Λ"^(0))^("—")$]], [1115.6], [#math.equation(block: false, alt: "2.6 times 10 to the power −10")[$2.6 #h(0.2em) × #h(0.2em) 10^(−10)$]], [], [Sigma], [#math.equation(block: false, alt: "Σ to the power plus")[$"Σ"^(+)$]], [#math.equation(block: false, alt: "Σ to the power −")[$"Σ"^("−")$]], [1189.4], [#math.equation(block: false, alt: "0.80 times 10 to the power −10")[$0.80 #h(0.2em) × #h(0.2em) 10^(−10)$]], [], [Xi], [#math.equation(block: false, alt: "Ξ to the power plus")[$"Ξ"^(+)$]], [#math.equation(block: false, alt: "Ξ to the power −")[$"Ξ"^("−")$]], [1315], [#math.equation(block: false, alt: "2.9 times 10 to the power −10")[$2.9 #h(0.2em) × #h(0.2em) 10^(−10)$]], [], [Omega], [#math.equation(block: false, alt: "Ω to the power plus")[$"Ω"^(+)$]], [#math.equation(block: false, alt: "Ω to the power −")[$"Ω"^("−")$]], [1672], [#math.equation(block: false, alt: "0.82 times 10 to the power −10")[$0.82 #h(0.2em) × #h(0.2em) 10^(−10)$]], [Mesons], [Pion], [#math.equation(block: false, alt: "π to the power plus")[$π^(+)$]], [#math.equation(block: false, alt: "π to the power −")[$π^("−")$]], [139.6], [#math.equation(block: false, alt: "2.60 times 10 to the power −8")[$2.60 #h(0.2em) × #h(0.2em) 10^(−8)$]], [], [#math.equation(block: false, alt: "π")[$π$]-Zero], [#math.equation(block: false, alt: "π to the power 0")[$π^(0)$]], [#math.equation(block: false, alt: "π to the power 0")[$π^(0)$]], [135.0], [#math.equation(block: false, alt: "0.83 times 10 to the power −16")[$0.83 #h(0.2em) × #h(0.2em) 10^(−16)$]], [], [Kaon], [#math.equation(block: false, alt: "K to the power plus")[$"K"^(+)$]], [#math.equation(block: false, alt: "K to the power −")[$"K"^("−")$]], [493.7], [#math.equation(block: false, alt: "1.24 times 10 to the power −8")[$1.24 #h(0.2em) × #h(0.2em) 10^(−8)$]], [], [#emph[k]-Short], [#math.equation(block: false, alt: "K S 0")[$"K"_(S)^(0)$]], [#math.equation(block: false, alt: "K S 0 —")[$accent("K"_(S)^(0), "—")$]], [497.6], [#math.equation(block: false, alt: "0.89 times 10 to the power −10")[$0.89 #h(0.2em) × #h(0.2em) 10^(−10)$]], [], [#emph[k]-Long], [#math.equation(block: false, alt: "K L 0")[$"K"_(L)^(0)$]], [#math.equation(block: false, alt: "K L 0 —")[$accent("K"_(L)^(0), —)$]], [497.6], [#math.equation(block: false, alt: "5.2 times 10 to the power −8")[$5.2 #h(0.2em) × #h(0.2em) 10^(−8)$]], [], [J#emph[/]#math.equation(block: false, alt: "ψ")[$ψ$]], [J#emph[/]#math.equation(block: false, alt: "ψ")[$ψ$]], [J#emph[/]#math.equation(block: false, alt: "ψ")[$ψ$]], [3100], [#math.equation(block: false, alt: "7.1 times 10 to the power −21")[$7.1 #h(0.2em) × #h(0.2em) 10^(−21)$]], [], [Upsilon], [#math.equation(block: false, alt: "Υ")[$"Υ"$]], [#math.equation(block: false, alt: "Υ")[$"Υ"$]], [9460], [#math.equation(block: false, alt: "1.2 times 10 to the power −20")[$1.2 #h(0.2em) × #h(0.2em) 10^(−20)$]], )) The same forces that hold ordinary matter together also hold antimatter together. Under the right conditions, it is possible to create antiatoms such as antihydrogen, antioxygen, and even antiwater. In antiatoms, positrons orbit a negatively charged nucleus of antiprotons and antineutrons. compares atoms and antiatoms. #figure(figph[Figure a shows a hydrogen atom and an antihydrogen atom. The former has a circle labeled p at the center and another, smaller circle labeled e minus in an orbit around it. The latter has a circle labeled p bar at the center and another, smaller circle labeled e plus in an orbit around it. Figure b shows a helium atom and an antihelium atom. The former has a circle labeled 2p 2n at the center and two smaller circles labeled e minus in an orbit around it. The latter has a circle labeled 2p bar 2 n bar at the center and two smaller circles labeled e plus in an orbit around it.], alt: "Figure a shows a hydrogen atom and an antihydrogen atom. The former has a circle labeled p at the center and another, smaller circle labeled e minus in an orbit around it. The latter has a circle labeled p bar at the center and another, smaller circle labeled e plus in an orbit around it. Figure b shows a helium atom and an antihelium atom. The former has a circle labeled 2p 2n at the center and two smaller circles labeled e minus in an orbit around it. The latter has a circle labeled 2p bar 2 n bar at the center and two smaller circles labeled e plus in an orbit around it.", caption: [A comparison of the simplest atoms of matter and antimatter. (a) In the Bohr model, an antihydrogen atom consists of a positron that orbits an antiproton. (b) An antihelium atom consists of two positrons that orbit a nucleus of two antiprotons and two antineutrons.]) Antimatter cannot exist for long in nature because particles and antiparticles annihilate each other to produce high-energy radiation. A common example is electron-positron annihilation. This process proceeds by the reaction #math.equation(block: true, alt: "e to the power − plus e to the power plus → 2 γ .")[$"e"^("−") + "e"^(+) → 2 γ .$] The electron and positron vanish completely and two photons are produced in their place. (It turns out that the production of a single photon would violate conservation of energy and momentum.) This reaction can also proceed in the reverse direction: Two photons can annihilate each other to produce an electron and positron pair. Or, a single photon can produce an electron-positron pair in the field of a nucleus, a process called pair production. Reactions of this kind are measured routinely in modern particle detectors. The existence of antiparticles in nature is not science fiction. #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ Watch this #link("https://openstax.org/l/21matter")[video] to learn more about matter and antimatter particles. ] === Summary - The four fundamental forces of nature are, in order of strength: strong nuclear, electromagnetic, weak nuclear, and gravitational. Quarks interact via the strong force, but leptons do not. Both quark and leptons interact via the electromagnetic, weak, and gravitational forces. - Elementary particles are classified into fermions and boson. Fermions have half-integral spin and obey the exclusion principle. Bosons have integral spin and do not obey this principle. Bosons are the force carriers of particle interactions. - Quarks and leptons belong to particle families composed of three members each. Members of a family share many properties (charge, spin, participation in forces) but not mass. - All particles have antiparticles. Particles share the same properties as their antimatter particles, but carry opposite charge. === Conceptual Questions What are the four fundamental forces? Briefly describe them. #solutionbox[ Strong nuclear force: interaction between quarks, mediated by gluons. Electromagnetic force: interaction between charge particles, mediated photons. Weak nuclear force: interactions between fermions, mediated by heavy bosons. Gravitational force: interactions between material (massive) particle, mediate by hypothetical gravitons. ] Distinguish fermions and bosons using the concepts of indistiguishability and exchange symmetry. List the quark and lepton families #solutionbox[ electron, muon, tau; electron neutrino, muon neutrino, tau neutrino; down quark, strange quark, bottom quark; up quark, charm quark, top quark ] Distinguish between elementary particles and antiparticles. Describe their interactions. === Problems How much energy is released when an electron and a positron at rest annihilate each other? (For particle masses, see .) #solutionbox[ 1.022 MeV ] If #math.equation(block: false, alt: "1.0 times 10 to the power 30 MeV")[$1.0 #h(0.2em) × #h(0.2em) 10^(30) #h(0.2em) "MeV"$] of energy is released in the annihilation of a sphere of matter and antimatter, and the spheres are equal mass, what are the masses of the spheres? When both an electron and a positron are at rest, they can annihilate each other according to the reaction #math.equation(block: true, alt: "e to the power − plus e to the power plus → γ plus γ .")[$e^("−") + e^(+) → γ + γ .$] In this case, what are the energy, momentum, and frequency of each photon? #solutionbox[ 0.511 MeV, #math.equation(block: false, alt: "2.73 times 10 to the power −22 kg times m / s")[$2.73 #h(0.2em) × #h(0.2em) 10^(−22) #h(0.2em) "kg" · "m" "/" "s"$], #math.equation(block: false, alt: "1.23 times 10 to the power 20 Hz")[$1.23 #h(0.2em) × #h(0.2em) 10^(20) #h(0.2em) "Hz"$] ] What is the #emph[total kinetic energy] carried away by the particles of the following decays? #linebreak() #math.equation(block: false, alt: "open parenthesis a close parenthesis π to the power 0 → γ plus γ; open parenthesis b close parenthesis K to the power 0 → π to the power plus plus π to the power −; open parenthesis c close parenthesis Σ to the power plus → n plus π to the power plus; open parenthesis d close parenthesis Σ to the power 0 → Λ to the power 0 plus γ .")[$( "a" ) #h(0.2em) π^(0) → γ + γ \ ( "b" ) #h(0.2em) "K"^(0) → π^(+) + π^("−") \ ( "c" ) #h(0.2em) Σ^(+) → n + π^(+) \ ( "d" ) #h(0.2em) Σ^(0) → Λ^(0) + γ .$]