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Transcript
Schwennesen 1
Fundamental Particles and the Physics of the Miniscule
Ben Schwennesen
Duke University
Professor Hubert Bray
Schwennesen 2
Fundamental Particles and the Physics of the Miniscule
Indivisibility: A Brief History of the Fairly Small
Since the time of the ancient Greeks (and perhaps even earlier), humanity has pondered
what components coalesce to form the world around us [1]. Not only have people questioned
what matter is formed from, further still, some of history’s greatest minds have sought to identify
the smallest parts that give form to everything [6, p. 47]. In other words, the concept of
indivisibility and to what objects it might apply is a perplexing one. To Plato, indivisibility was
a question of geometry: the four objects essential to all matter (which Greeks, including Plato,
considered categorically as incarnations of the four elements—fire, earth, air, and water)
corresponded to the tetrahedron, cube, octahedron, and icosahedron [2]. Indeed, the word
“atom” was derived from the Greek philosophy of atomism, since the atom was considered
fundamental and indivisible upon its discovery (though the atom is now known to be
devastatingly divisible, as demonstrated by the Manhattan Project) [1]. The work of scientists
like John Dalton, J.J. Thomson, Ernest Rutherford, Niels Bohr, Erwin Schrödinger, and Werner
Heisenberg throughout the 19th and 20th centuries brought about a conversion of the atomist
philosophy into a full-fledged atomic theory [7]. Experiments in this field led to the discovery of
previously unknown particles—particles far smaller than the proton and neutron—giving birth to
the Standard Model of particle physics.
The “Spin” of Fundamental Particles
In order to understand the particles of the Standard Model, one must first understand the
characteristics used to describe these particles. The angular momentum of a particle is defined in
the same way one would define the angular momentum of a macroscopic object: it is the product
Schwennesen 3
of its inertia to rotation (a function of the object’s mass distribution relative to the axis of
rotation) and its spin velocity (which is proportional to the number of rotations per unit of time)
[6, p. 29]. Since angular momentum is a vector quantity, magnitude is not the only information
it carries: the direction of angular momentum is defined as being orthogonal to the plane of
rotation; thus, if an observer saw a particle rotating clockwise, the particle’s angular momentum
would be directed away from this observer [6, p. 30].
Angular momentum came to be identified as an intrinsic aspect of fundamental particles
through experiments testing the Zeeman effect, in which a magnetic field affects the energy of a
photon released when electrons jump from one orbit around the nucleus to another (an aspect of
Bohr’s atomic model, in which angular momentum is quantized) [6, p. 31]. After many years of
experiments, the Zeeman effect was found to result in changes in energy that contradicted Bohr’s
integer value orbital model; instead, as the two graduate students George Uhlenbeck and Samuel
Goudsmit proposed in 1925, the quantum number describing an electron’s angular momentum is
a half-integer multiplied by ħ (“h-bar”, equal to Planck’s constant divided by 2π). Along any
given axis, therefore, an electron’s rotation about itself could only appear as spin up, + ħ/2, or
spin down, - ħ/2 (most physicists will set ħ equal to unity, so that the spins appear as ±1/2) [6, p.
31]. As explained by Wolfenstein and Silva, however, it is vital that one recognizes that “this
internal rotation [spin] is just a mental picture, physical rotation does not make sense for
fundamental point-like particles” [p. 31]. Crucially, when combined with the orbital angular
momentum, the spin gives the total angular momentum, which is a conserved quantity in any
particle interaction [6, p. 32].
The sign of a particle’s spin is determined by a measure known as helicity, defined as the
projection of the particle’s spin along its direction of motion. A particle with spin pointing along
Schwennesen 4
the direction of motion has positive helicity, while spin against the direction of motion indicates
negative helicity; by convention, physicists tend to call particles with positive helicity righthanded and those with negative helicity left-handed [6, p. 32]. The helicity of a particle is
closely related to another measure, called chirality, which was developed in the context of
massive particles [6, p. 81].
For massless particles, most famously photons, chirality is identical to helicity, as the
helicity of the particle is, by necessity, a relativistic invariant: the helicity is the same in all
reference frames because no frame may exceed the speed of the photon [6, p. 33]. By contrast,
massive particles may travel slower than the reference frame of some observer, such that a
particle with positive helicity will appear to have negative helicity to the observer in the fast
moving frame; hence, helicity is frame-dependent [6, p. 33]. For an object, macroscopic or
otherwise, to have chirality, its mirror image must not be identical to itself [3]; hence, in the
context of particle physics, massive particles fit this description since they appear to have
different helicity when viewed from different frames of reference. The result of this phenomena
was striking to physicists: only left-handed chiral fermions and right-handed chiral antifermions
participate in the weak interaction; despite the invariance of physical processes under
transformations, one interaction occurs and its parity transformation does not [6, p. 81], implying
that the Universe does not have parity (positive-negative) symmetry [3].
Fermions: Leptons
The Standard Model electron is of a type of particle called a fermion (after Enrico Fermi),
all of which have half integer spin; all particles that make up matter are fermions [6, p. 31].
Specifically, electrons are part of the class of fermions known as leptons, distinguished from
other the other class of fermions, known as quarks, in that they do not participate in the strong
Schwennesen 5
interaction (more on this later) [0, pg. 70]. Three generations of leptons exist, with two particles
in each generation: the first in each pair is charged while the second is not. The first generation
leptons, the electron and electron-neutrino (e & νe), are found commonly in nature [0, p. 70].
The muon and the muon-neutrino (μ & νμ) make up the second generation, and are also fairly
natural observations, at least in certain environments. The third and final generation, consisting
of the tau and tau-neutrino (τ & ντ), have only been observed in laboratories [0, p. 71]. Neutrinos
are exceptionally elusive particles due to their lack of charge and extremely low mass: detection
of a particle that will not respond outright to electromagnetism and the strong force (and
effectively not to gravitation, either) is incredibly difficult. As such, in order to significantly
impede the approximate 1012 electron neutrinos that pass through any given human’s body every
second, one would need a block of lead “ninety thousand million million meters thick” [0, pg.
74].
There is an advantage to the elusive nature of the neutrinos in that they allow particle
physicists to study the weak interaction in an uncluttered manner. Though the probability of
their reactions are miniscule, they are plentiful enough that reactions are not excessively difficult
to study [0, p. 74]. A canonical example of a reaction involving neutrinos is given by:
𝜈𝑒 + 𝑛 → 𝑝 + 𝑒 − ,
where n is a neutron and p is a proton. An example of this reaction where the neutron is
contained in an atom is [0, p. 74]:
37
17𝐶𝑙
+ 𝜈𝑒 →
37
18𝐴𝑟
+ 𝑒−.
To understand how the neutron in this reaction is changed into a proton, one must first
understand another type of fermion—quarks.
Schwennesen 6
Fermions: Quarks
Quarks were first identified by experiments involving pions (π+, π0, or π-), which were
only understood at the time as particles that mediated the conversion of protons to neutrons and
vice versa [6, p. 53]. In 1964, Murray Gell-Mann and George Zweig independently published
proposals which argued that protons and neutrons were in fact composite particles made up of
some as-yet unidentified fundamental particles; Gell-Mann was responsible for the name
“quark,” derived from James Joyce’s Finnegans Wake [6, p. 58].
Soon, it became clear that
protons and neutrons consisted of three quarks each (any particle of this composition is known as
a baryon [6, p. 60]), inexorably bound together by the strong interaction. The two “flavors”
(types) of quarks found in protons and neutrons are the up quark (u), with a charge of +2/3, and
the down quark (d), with a charge of -1/3. Hence, since there must be a +1 charge on the proton
and no charge on the neutron, the proton consists of two up and one down quark (p = uud) while
the neutron consists of one up and two down quarks (n = udd) [6, p. 58]. Pions, furthermore,
came to be seen as the combination of a quark with an antiquark—i.e. the antimatter counterpart
of a quark (π+ = u𝑑,
𝜋 0 = 𝑑𝑑 − 𝑢𝑢, 𝜋 − = 𝑢𝑑) [6, p. 58]. (To be consistent with relativity,
the production of a corresponding antiparticle for each known particle must be possible in the
Universe, though they need not exist simultaneously. Indeed, when particles and antiparticles
are close enough to interact, they undergo annihilation reactions which release massive amounts
of energy and sometimes produce exotic particles [0, p. 99].) Any particle composed of a quark
and an antiquark, like the pion, is called a meson; baryons and mesons are considered types of
hadrons, any composite particle of quarks bound together by the strong interaction [6, p. 62].
The formulation of the pion as a meson allows for explanation of the neutrino reaction
described earlier: to convert a neutron to a proton, a d quark must be changed into a u [0, p. 75].
Schwennesen 7
Pions most commonly decay into muon/muon antineutrino pairs or antimuon/muon neutrino
pairs, due to the favorable helicity of these particles (i.e., due to the Universe’s lack of parity
symmetry on the scale of fundamental particles [6, p. 81]). These or corresponding first
generation lepton pairs, which are less likely but still possible decay products, lead to the
conversion of the d quark into a u (or vice-versa) via the weak interaction [6, p. 59; 0, p. 76]:
𝜈𝜇 + 𝑑 → 𝑢 + 𝜇 −
&
𝜈𝑒 + 𝑑 → 𝑢 + 𝑒 − .
These reactions demonstrate a crucial rule in particle physics, the conservation of electrical
charge: any reaction must preserve the total charge of all particles [0, p. 76]. In the above
examples, the left hand sides of the equations have total charge of -1/3, all from the down quark,
while the right hand sides have -1/3 total charge, with +2/3 from the up quark and -1 from the
electron, i.e., (0) + (-1/3) = (+2/3) + (-1) [0, p. 76].
There are four other flavors of quarks aside from those found in baryonic matter, which
form generations similar to those of the leptons (with u and d being the first generation): the
charm (c) and strange (s) quarks form the second generation, while the top (t) and bottom (b)
quarks constitute generation three [0, p. 107]. These generations are distinct from those of the
leptons, however, in that they are identified by flavor numbers (U = 1 & D = -1, C = 1 & S = -1,
T = 1 & B = -1). (Note that the flavor numbers of antiquarks are the same but with opposite
parity [0, p. 107].) These other flavors lead to other composite particles, though they are rarely
observed in nature [0, p. 111].
The Behavior of Particles and Quantum Field Theory
One of the key developments of science in the 20th century was the recognition that
electrons and photons (eventually encompassing all particles, as well) have both wave-like and
Schwennesen 8
particle-like properties; as such, they are now regarded as quanta [6, p. 37]. Mathematically,
quanta may be described using the framework of quantum field theory (QFT), which Wolfenstein
and Silva laud as “the consistent theory joining quantum mechanics and special relativity” [6, p.
37]. Each quanta is described by its own quantum field; the consistent QFT of electron and
photon fields, quantum electrodynamics (QED), was put forth by Richard Feynman, Julian
Schwinger, and Sin-Itiro Tomonaga in the mid-20th century. QED describes the nature of
interactions between electrons and photons, and though precise details about the theory would be
enough to fill entire books, the introduction of Feynman diagrams allowed its ideas to be
communicated in terms far simpler than the actual mathematics behind them (see Figure 1 for an
example) [6, p. 38]. Similar QFTs which emerged later arguably owe their credibility to the
elegance of the model laid out by Feynman and the other pioneers of QED [0, p. 202].
Figure 1: Feynman diagram representing a second-order
interaction, specifically electron-electron scattering
Retrieved from:
http://chemphys.armstrong.edu/secrest/Astro/astro_1.html
Feynman’s contributions to particle physics are not limited to his contributions to QED.
In his work on the fairly well-known double slot experiment for electrons, Feynman could not
relate to the contemporary methods of doing quantum mechanical calculations, so he developed a
“beautifully elegant” method for describing probabilities in interactions on the smallest scale [0,
p. 50]. The essence of the experiment is that quantum probabilities are not additive: when
opening one of two slots to allow electrons to pass through, then opening only the other in
another trial, and finally opening both simultaneously, the distribution of electrons in the final
Schwennesen 9
trial does not correspond to a summation of the first two, as would be expected macroscopically
[0, p. 49]. Feynman proposed that the probability of an event on the quantum scale is related to a
quantity in the complex field called the amplitude. To calculate the probability of travelling
from a to b, one must add the amplitude of each possible path (no matter how unlikely) and take
the absolute square [0, p. 51]:
probability(a,b) = |Amp(a,b)path 1 + Amp(a,b)path 2 + … + Amp(a,b)path n |2
Bosons and the Fundamental Forces
Bosons (after Satyendra Bose), the second top-level classification in the Standard Model,
are particles with integer spin (including zero); bosons are the force carriers for the fundamental
interactions [6, p. 31]. Wolfenstein and Silva assert that one of the greatest achievements of
particle physics to date was the narrowing of unthinkable numbers of phenomena down to their
root in the four fundamental forces, all of which may be described mathematically [6, p. 109].
Each fundamental force is relevant at different scales. Gravity is significant only on the
macroscopic level, as it is so very weak: the strength of the electromagnetic force—the best
understood of the fundamental interactions—divided by the force of gravity is a massive number,
1036 (if this number were smaller, the cosmos would be far less vast and very short lived) [4, p.
2]. As described earlier, the theory of QED is a highly successful model of the electromagnetic
force, which acts from the planetary scale all the way down to quarks and leptons [6, p. 110].
Models similar to QED have emerged to describe the strong and weak interactions, which
are relevant only on the subatomic scale [6, p. 111]. Quantum chromodynamics (QCD) is the
theory that emerged to describe the strong force between quarks; though QCD is similar to QED
in outline, the mathematics of QCD is more difficult to utilize in practice, as the theory is not
Schwennesen 10
‘well-behaved’ and models actually become more important with increasing complexity
(whereas in QED, increasingly complex Feynman diagrams are less important to total amplitude)
[0, p. 203]. QCD earned its name by explaining quarks as having three distinct ‘strong charges,’
deemed ‘colors,’ in analogy with the three primary colors [6, p. 115]. A fascinating property of
QCD explains why isolation of an individual quark in nature is thought impossible: as the
distance between quarks increases, so does the force between them [0, p. 203]. Thus, as one tries
to pull out a single quark (or gluon, to be discussed below), the energy in the quantum field
between them becomes so great that a particle-antiparticle pair will appear instead and form new
hadrons [6, p. 116].
Finally, the weak interaction model was developed to explain certain decays which could
not be explained by any of the other three forces [6, p. 111]. In attempting to develop a formal
theory for the weak interaction, its properties were found to be so similar to QED that it was
possible to develop a single mathematical theory describing both forces, which came to be
known as electroweak theory [0, p. 204]. The unification of these two forces is counterintuitive,
as they act over entirely different ranges: electromagnetism essentially has an unbounded range,
while the weak interaction is constrained to scales less than 10-18 meters [0, p. 204]. Since the
weak field suggested by electroweak theory acted identically to the electromagnetic field, an
explanation for this short range was necessarily to come from some new aspect of particle
physics; this explanation turned out to be the only scalar field in the Standard Model, the Higgs
field, which was found to interact with each of the other fields (all of which are either gauge or
tensor fields) [0, p. 205].
Each fundamental interaction is mediated by a force-carrying particle (though for
gravitation this particle remains hypothetical). Exchange particles, described precisely, are
Schwennesen 11
actually disturbances of the given force’s field caused by interactions between particles subject
to the force [0, p. 208]. The most well-known of these force carriers is the photon, the mediator
of the electromagnetic force, which has zero mass and travels at the speed of light [6, p. 114].
The exchange particles for the strong interaction are a set of eight massless particles known as
gluons. Since gluons are also subjects to the strong force they carry, individual gluons cannot be
isolated from the strong field [6, p. 115]. For the weak field, it turns out that three types of
disturbances exist, all of which have mass: the W+ and W- bosons, which form a particleantiparticle pair (as they have opposite electric charges and equal mass), and the neutral Z boson.
The mass of the Z boson is about 13% greater than the W bosons, which are, in turn, about 85
times the mass of a proton [6, p. 115]. In principle, all the exchange particles are massless, but
the interactions of the W and Z bosons with the Higgs field grant them large masses [0, p. 208].
Though gravitation in Einstein’s theory of general relativity is suspected to be quantized, as with
the other forces, which would imply a massless force-carrier due to gravity’s infinite range
(deemed the graviton), no predictive theory of quantum gravity has emerged [6, p. 117].
Conclusion: The Large Hadron Collider and the Power of Experimentation
Many of the particles described by the Standard Model are only known to exist through
experiments that subject ordinary particles to extremely high energies, usually by means of highspeed collisions. The Large Hadron Collider (LHC) is a circular facility, 27 km long,
constructed at CERN (Conseil Européen pour la Recherche Nucléaire) in Geneva, Switzerland
[6, p. 215; 0, p. 191]. The LHC replaced another project at CERN, the LEP (Large ElectronPositron) collider; according to Wolfenstein and Silva, the LHC can “accelerate protons to
99.9999991% of the speed of light” [p. 215]. Collisions between these rapidly moving protons
occur about 600 million times per second at four sites around the facility, each with their own
Schwennesen 12
detectors: ATLAS, CMS, LHCb, and ALICE; the former two are devoted to finding the elusive
Higgs boson. Curving the paths of the protons requires special superconducting magnets
operating at around -271 degrees Celsius [6, p. 215]. To store the data from all the collisions
(estimated to be about 15 million gigabytes per year), CERN had to establish an international
network of computers to share the load, which came to be called ‘the Grid’ [6, p. 216].
The amounts of technology crammed into the LHC is almost incomprehensible, all for
the sake of knowledge of a world so small we can never truly understand it. After decades of
construction, planning, and anticipation, CERN announced that it had finally identified the Higgs
boson at a mass of about 125 giga-electron volts (GeV); in 2013, Peter Higgs and François
Englert were awarded the Nobel Prize in physics for their original proposals of the Higgs
mechanism [5]. The mass of 125 GeV, as it turned out, left physicists with many questions:
since “no evidence for supersymmetry or for any competing ideas—such as “technicolor” and
“warped extra dimensions”—turned up during the first run of the LHC from 2010 to 2013,” new
theories of particle physics were mandated by the Higgs [5]. The hope of many theorists is that
further experiments at higher energies will reveal evidence for some theory of quantum gravity,
as opposed to the virtual dead end supplied by the multiverse theory [5]. For now, however,
particle physicists can rest peacefully, knowing that the mass of the Higgs boson at 125 GeV
does not complete the Standard Model, and therefore new physics is still out there waiting to be
discovered.
Schwennesen 13
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[4]
Rees, M. J. (2000). Just Six Numbers: The Deep Forces that Shape the Universe. New York:
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[5]
Wolchover, N. (2015, June 6). A New Theory to Explain the Higgs Mass. Retrieved February
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Wolfenstein, L., & Silva, J. P. (2011). Exploring Fundamental Particles. Boca Raton, FL: CRC
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[7]
Zheng, A. (2012, July-December). The Evolution of Atomic Theory. Young Scientists Journal,
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