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Open CosmologyPhysics & cosmology: four years, plus a graduate year

The Standard Model, gauge theories and grand unification

The third problem of the conventional Big Bang, magnetic monopoles, only arises in grand unified theories. To get there, Guth sketches the Standard Model of particle physics, why nobody thinks it is final, what a gauge theory is, and how SU(5) contains SU(3) × SU(2) × U(1).

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Full reading path (40 pages)
  1. Vectors (8.01)
  2. Position and velocity in one dimension (8.01)
  3. Acceleration in one dimension (8.01)
  4. Motion in two dimensions and projectiles (8.01)
  5. The homogeneous expanding universe (8.286)
  6. The Doppler effect and special relativity (8.286)
  7. Cosmological redshift (8.286)
  8. Newton's laws of motion (8.01)
  9. The universal law of gravitation (8.01)
  10. Why a static universe cannot work (8.286)
  11. The expanding sphere and the equation for a(t) (8.286)
  12. The Friedmann equation (8.286)
  13. Open, closed and flat universes (8.286)
  14. The closed universe as a cycloid (8.286)
  15. The age of the universe and the Big Bang singularity (8.286)
  16. The age of a closed universe from H and Ω (8.286)
  17. The open universe and the age of any matter universe (8.286)
  18. Non-Euclidean geometry (8.286)
  19. The metric of a sphere and of a closed universe (8.286)
  20. Curvature and expansion — the Robertson–Walker metric (8.286)
  21. The geometry of open universes (8.286)
  22. The spacetime interval (8.286)
  23. The spacetime metric of the universe (8.286)
  24. The geodesic equation (8.286)
  25. Simplifying the geodesic equation (8.286)
  26. Falling into a black hole (8.286)
  27. Mass, energy and the dilution of radiation (8.286)
  28. Matter–radiation equality and the pressure of light (8.286)
  29. The horizon distance (8.286)
  30. The radiation-dominated universe (8.286)
  31. The cosmological constant and vacuum energy (8.286)
  32. The age of the universe with vacuum energy (8.286)
  33. How bright is a distant supernova? (8.286)
  34. The supernova evidence for acceleration (8.286)
  35. The puzzle of the vacuum energy, and Einstein's mistake about Friedmann (8.286)
  36. Black-body radiation (8.286)
  37. Neutrinos and counting particle species (8.286)
  38. The temperature of the early universe and decoupling (8.286)
  39. The horizon problem (8.286)
  40. The flatness problem (8.286)
On this page · 5 sections
  1. The Standard Model of particle physics
  2. Gauge theories
  3. SU(3) × SU(2) × U(1)
  4. Grand unification: SU(5)
  5. Summary

The third problem of the conventional Big Bang is the magnetic monopole problem. Unlike the horizon and flatness problems, it is not a problem of classical cosmology. It arises only if physics at very high energies is described by grand unified theories, which predict magnetic monopoles and let us estimate how many the early universe would have made — far too many, without inflation. If you don't believe in grand unified theories, which you are allowed not to, the problem goes away; but there is some evidence for them.

Guth can't teach grand unified theories in ten minutes, so he collects enough facts to make a consistent picture. He runs out of time before reaching the monopoles themselves; the discussion continues in Lecture 22.

The Standard Model of particle physics#

The Standard Model, developed since the 1970s, has changed little since about 1975. The main later addition is that neutrinos have masses, which can be incorporated.

Guth shows the familiar chart of its particles (slide 6, from Wikimedia Commons; a version in words follows):

Generation IGeneration IIGeneration III
Quarks (charge +2/3)upcharmtop
Quarks (charge −1/3)downstrangebottom
Neutrinoselectron neutrinomuon neutrinotau neutrino
Charged leptonselectronmuontau
  • Spin-½ particles (fermions) fall into three generations. There are six flavours of quark, and each comes in three colours. The colours are perfectly symmetric — absolutely identical — while the flavours all differ, with only approximate symmetries between them. With each family of quarks goes a family of leptons, particles without strong interactions: a neutrino and an electron-like particle.
  • Spin-1 particles (gauge bosons): the photon of electromagnetism; the gluon, which plays the photon's role for the strong interactions, which are more complicated; and the Z⁰ and W±, carriers of the weak interactions — the only non-gravitational interactions neutrinos feel. A weak process example is neutron decay, n→p+e−+νˉen \to p + e^- + \bar\nu_e, where the antineutrino balances electron lepton number. Essentially anything involving neutrinos is a weak interaction.
  • The chart Guth shows predates 2012 and leaves out the Higgs boson, the spin-0 particle of the Higgs field, found at CERN in 2012; it completes the Standard Model, and the Higgs field is the subject of Lecture 22.

With its interactions this is a complete model of how elementary particles behave, and it agrees with every reliable experiment since the mid-1970s. That has made particle physics a bit dull, Guth jokes, but it is a magnificent achievement.

Why nobody thinks it is final

Guth knows nobody who regards the Standard Model as a candidate for the ultimate theory:

  1. It does not include gravity, and there is no simple way to add it.
  2. It has no good candidate for the dark matter.
  3. It has about 28 free parameters — numbers that must be measured before it predicts anything. That is only an aesthetic argument, but theorists take it seriously: many parameters mean ugliness, and almost all expect the true theory to have far fewer adjustable knobs, perhaps none.

Why is the strong force short-ranged?

A student asks: the weak force is short-ranged because the W and Z are very heavy, but the strong force is short-ranged too, and the gluon is effectively massless. The answer is confinement. Gluons cannot exist as free particles. In a sense the strong force is long-ranged: pull apart a meson, a quark and an antiquark, and a "string" of gluon force between them pulls with a constant force however far you go. What intervenes is that, stretched far enough, it becomes energetically favourable for a new quark–antiquark pair to appear in the middle. The string breaks into two shorter strings, each with a quark at one end and an antiquark at the other — but a string can never simply end in empty space. At very short distances gluons behave like ordinary particles; at larger distances confinement dominates.

Gauge theories#

Grand unified theories grow out of the Standard Model through the idea of a gauge theory: a theory in which the fields are not themselves reality. There is a set of transformations that take one field configuration to another describing the same physical situation, so many field configurations correspond to one reality.

The example you know is electromagnetism. Writing the fields in terms of potentials,

Fields from potentials
E⃗=−∇⃗ϕ−1c∂A⃗∂t,B⃗=∇⃗×A⃗,Aμ=(−ϕ,Ai)\vec E = -\vec\nabla\phi - \frac{1}{c}\frac{\partial\vec A}{\partial t}, \qquad \vec B = \vec\nabla\times\vec A, \qquad A_\mu = (-\phi, A_i)
In words

vector E equals minus vector del phi minus 1 over c partial vector A over partial t , vector B equals vector del cross vector A , A sub mu equals (- phi , A sub i )

Source: 8.286 Lecture 21 slides, slide 7

for any function Λ(t,x⃗)\Lambda(t, \vec x) one may replace

Gauge transformation
ϕ′(t,x⃗)=ϕ−1c∂Λ∂t,A⃗′(t,x⃗)=A⃗+∇⃗Λ,Aμ′(x)=Aμ(x)+∂Λ∂xμ\phi'(t,\vec x) = \phi - \frac{1}{c}\frac{\partial\Lambda}{\partial t}, \qquad \vec A'(t,\vec x) = \vec A + \vec\nabla\Lambda, \qquad A'_\mu(x) = A_\mu(x) + \frac{\partial\Lambda}{\partial x^\mu}
In words

phi prime (t, vector x ) equals phi minus 1 over c partial lambda over partial t , vector A prime (t, vector x ) equals vector A plus vector del lambda , A prime sub mu (x) equals A sub mu (x) plus partial lambda over partial x superscript mu

Source: 8.286 Lecture 21 slides, slide 7

and E⃗\vec E and B⃗\vec B — which contain all the physics — are unchanged. [The slide writes ϕ′=ϕ−∂Λ/∂t\phi' = \phi - \partial\Lambda/\partial t; with E⃗\vec E defined as above, and x0=ctx^0 = ct in the covariant form, the factor 1/c1/c is needed.] All the important field theories we know are gauge theories.

Two successive gauge transformations must again be a symmetry, so it matters how they combine. In electromagnetism they simply add:

Combining gauge transformations
Λ3=Λ1+Λ2\Lambda_3 = \Lambda_1 + \Lambda_2
In words

lambda sub 3 equals lambda sub 1 plus lambda sub 2

Source: 8.286 Lecture 21 slides, slide 7

so the group is Abelian (commutative).

The crucial generalisation is to non-Abelian gauge theories, introduced by Yang and Mills in 1954. Nobody knew what to do with them at first, but they became the Standard Model. Here the gauge parameter is an element of a group, and successive transformations multiply according to that group's rules.

SU(3) × SU(2) × U(1)#

The Standard Model uses three gauge groups — itself an example of its ugliness, and a source of extra parameters:

  • SU(3): the 3×33 \times 3 matrices that are unitary, U†U=1U^\dagger U = 1, and special, with determinant 1.
  • SU(2): the same with 2 in place of 3.
  • U(1): the group of phases eiϕe^{i\phi} — complex numbers of magnitude 1.

The three act independently, so the full gauge group is the product group SU(3) × SU(2) × U(1): an element is just one element of each, written together.

Grand unification: SU(5)#

A grand unified theory embeds these three groups in a single simple group (a term with a precise meaning in group theory, but "simple" in the everyday sense will do here). The first one invented uses SU(5), the 5×55 \times 5 unitary matrices of determinant 1. The embedding is easy:

  • put an SU(3) matrix in the upper-left 3×33 \times 3 block;
  • put an SU(2) matrix in the lower-right 2×22 \times 2 block;
  • for the U(1), give each block an overall phase: multiply the whole upper 3×33 \times 3 block by e2iϕe^{2i\phi} and the whole lower 2×22 \times 2 block by e−3iϕe^{-3i\phi}.

The phases are chosen so the determinant stays 1: (e2iϕ)3(e−3iϕ)2=e6iϕ−6iϕ=1(e^{2i\phi})^3(e^{-3i\phi})^2 = e^{6i\phi - 6i\phi} = 1. [The transcript says "the product of the five phases is 0"; it is the sum of their exponents that vanishes, so the product is 1.] Any SU(3) matrix, SU(2) matrix and angle ϕ\phi together give an SU(5) matrix, and the three pieces commute with one another, so SU(5) contains SU(3) × SU(2) × U(1) as a subgroup. That is how the simplest grand unified theory works.

Worked example

Checking the SU(5) embedding

Show that the block matrix M=diag(e2iϕU3, e−3iϕU2)M = \text{diag}(e^{2i\phi}U_3,\ e^{-3i\phi}U_2), with U3∈U_3 \in SU(3) and U2∈U_2 \in SU(2), lies in SU(5), and that its three ingredients commute.

Unitary

M†M=diag(U3†U3, U2†U2)=diag(13,12)=15M^\dagger M = \text{diag}(U_3^\dagger U_3,\ U_2^\dagger U_2) = \text{diag}(1_3, 1_2) = 1_5, because the phases have magnitude 1.

Determinant 1

det⁡M=(e2iϕ)3det⁡U3⋅(e−3iϕ)2det⁡U2=e6iϕe−6iϕ⋅1⋅1=1\det M = (e^{2i\phi})^3\det U_3 \cdot (e^{-3i\phi})^2\det U_2 = e^{6i\phi}e^{-6i\phi} \cdot 1 \cdot 1 = 1.

Commuting

The SU(3) piece acts only on the first three entries and the SU(2) piece only on the last two, so they commute. The U(1) piece is a multiple of the identity on each block, so it commutes with both. The product of an SU(3), an SU(2) and a U(1) element is therefore well defined in any order.

Guth ends here — out of time, he withholds the grand-unified-theory problem from the problem set, and the monopole discussion is picked up in the next lecture, which Guth says Scott Hughes will give.

Summary#

  • The magnetic monopole problem exists only if grand unified theories are right.
  • The Standard Model: three generations of quarks (six flavours, three colours each) and leptons, plus the photon, gluon, W± and Z⁰. It fits every reliable experiment since the mid-1970s, but lacks gravity and a dark matter candidate, and has about 28 free parameters.
  • Confinement explains the short range of the strong force despite massless gluons.
  • In a gauge theory many field configurations describe the same physics; electromagnetism is Abelian (Λ3=Λ1+Λ2\Lambda_3 = \Lambda_1 + \Lambda_2), while Yang–Mills theories are non-Abelian.
  • The Standard Model gauge group SU(3) × SU(2) × U(1) fits inside SU(5), the first grand unified theory.

Symbols on this page

Show the 16 symbols used here
Λ\Lambda capital lambda
The function in a gauge transformation. Say it: “lambda”.
μ\mu mu
A spacetime index, running over 0 (time) and 1, 2, 3 (space). Say it: “mu” (sounds like “myoo”).
ν\nu nu
A neutrino (T_ν, g_ν); ν̄ is an antineutrino. Say it: “nu” (sounds like “new”).
π\pi pi
The ratio of a circle's circumference to its diameter, π ≈ 3.14159. Say it: “pi”.
ϕ\phi phi
A phase angle; in A_μ = (−φ, A) it is the electric potential. Say it: “phi” (sounds like “fye”).
∈\in element of
Is an element of (belongs to) a set. Say it: “is in”.
→\to arrow
Goes to (tends to), or becomes. Say it: “goes to”.
×\times times
Times (multiplication). Between two vectors: the cross product. Say it: “times”.
⋅\cdot dot
Times (multiplication). Between two vectors: the dot product. Say it: “times”.
†\dagger dagger
Conjugate transpose of a matrix: transpose it and take complex conjugates (U†). Say it: “dagger”.
∂\partial partial
Partial derivative: the rate of change with one variable, holding the others fixed. Say it: “partial”.
∇\nabla nabla (del)
Del: ∇f is the gradient, ∇·v the divergence, ∇×v the curl, ∇² the Laplacian. Say it: “del”.
det⁡\det determinant
Determinant of a matrix. Say it: “the determinant of”.
v⃗\vec v vector arrow
A vector: a quantity with a size and a direction. Say it: “vector”.
ρˉ\bar\rho bar
An antiparticle (ν̄, x̄). Say it: “bar”.
cc c
The speed of light, c ≈ 2.998 × 10⁸ m/s. Say it: “c”.

Tap or click a symbol in a formula to see the same explanation. All symbols: symbols and notation.

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Check your understanding

  1. Why does the magnetic monopole problem differ from the horizon and flatness problems?
  2. Which is NOT one of Guth's reasons for doubting that the Standard Model is the final theory?
  3. The gluon is effectively massless, so why is the strong force short-ranged?
  4. What makes a gauge theory non-Abelian?
  5. In the SU(5) embedding, why does the U(1) phase appear as e2iϕe^{2i\phi} on three diagonal entries and e−3iϕe^{-3i\phi} on two?
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