CONFIDENTIAL
BSM-DRAFT
REV. 2026.05
VOL III — DECK 02 — BLUEPRINT

PARTICLE
PHYSICS

Working drawings for the smallest things. The Standard Model is the most precisely tested theory in human history — and it is incomplete.

P. 01 / 18 — OVERVIEW

The Standard Model.

Twelve fermions, four gauge bosons, one Higgs scalar. SU(3)C × SU(2)L × U(1)Y. Constructed piece by piece from the 1950s through the 1970s; verified, decimal by decimal, ever since.

up
u
2.16 MeV
charm
c
1.27 GeV
top
t
172.7 GeV
photon
γ
0
down
d
4.67 MeV
strange
s
93 MeV
bottom
b
4.18 GeV
gluon
g
0
electron
e
0.511 MeV
muon
μ
105.7 MeV
tau
τ
1.777 GeV
Z boson
Z
91.2 GeV
e-neutrino
νe
< 0.8 eV
μ-neutrino
νμ
< 0.19 MeV
τ-neutrino
ντ
< 18.2 MeV
W boson
W±
80.4 GeV
Higgs
H
125.25 GeV

FIG. 01 · STANDARD MODEL — THREE GENERATIONS, FOUR FORCES, ONE HIGGS

P. 02 / 18 — FORCES

Four fundamental forces.

Strong

Mediator: 8 gluons. Range: ~1 fm. Coupling αs ≈ 0.118 at MZ. Confines quarks; binds protons and neutrons via residual force.

Electromagnetic

Mediator: photon (massless). Infinite range. Coupling α ≈ 1/137. Holds atoms together; carries light, chemistry, electricity.

Weak

Mediator: W±, Z0. Range: ~10⁻¹⁸ m. Drives β-decay, neutrino interactions, hydrogen → helium fusion in the Sun.

Gravity

Hypothetical graviton (spin-2). Infinite range. ~10⁴⁰× weaker than EM. Quantum description: still missing.

P. 03 / 18 — LAGRANGIAN

The master equation.

The Standard Model Lagrangian, schematically:

ℒ = −¼ FμνFμν + i ψ̄ γμDμ ψ + ψ̄i yij ψj ϕ + |Dμ ϕ|2V(ϕ)

Term by term:

  • −¼ F²Gauge boson kinetic terms
  • iψ̄γᵘDμψFermion kinetic + interactions
  • ψ̄ y ψ ϕYukawa couplings → fermion masses
  • |Dϕ|²Higgs kinetic / gauge interaction
  • V(ϕ)Higgs potential — the Mexican hat

Mexican-hat Potential

v ≈ 246 GeV V(ϕ) = μ² |ϕ|² + λ|ϕ|⁴

Spontaneous symmetry breaking → mass

P. 04 / 18 — HIGGS

The Higgs mechanism.

1964: Peter Higgs, François Englert, Robert Brout, and others propose a scalar field whose nonzero vacuum expectation value gives mass to the W and Z bosons (and, via Yukawa coupling, to fermions). The photon stays massless.

2012: ATLAS and CMS at the LHC announce a 125 GeV scalar — the Higgs boson — at 5σ. Higgs and Englert share the 2013 Nobel.

Without it, electroweak symmetry would be unbroken, electrons would be massless, atoms would not exist, and you would not be reading this.

Higgs Decay Channels

H b b̄ — 58.4 % W W* — 21.5 % gg — 8.2 % τ τ — 6.3 % γ γ — 0.23 %

Branching ratios at mH = 125 GeV

P. 05 / 18 — FEYNMAN DIAGRAMS

Drawing interactions.

Richard Feynman, 1949. Time runs left to right. Straight lines: fermions (arrows show particle direction). Wavy: photons. Curly: gluons. Dashed: scalars. Each vertex carries a coupling constant.

e⁻ e⁻ scattering

γ e⁻ e⁻

Beta decay (n → p + e⁻ + ν̄)

d u W⁻ e⁻ ν̄ₑ

Higgs production by gluon fusion

t loop H g g
CERN
P. 06 / 18 — ACCELERATORS

Machines that see the small.

To probe distance d, you need wavelength < d; for matter waves, that means momentum > ħ/d. To resolve 10⁻¹⁹ m you need TeV scales. Hence the LHC.

CERN's Large Hadron Collider is a 26.7 km synchrotron under the Franco–Swiss border. Two counter-rotating proton beams collide at 13.6 TeV in the ATLAS, CMS, ALICE, and LHCb detectors.

  • Circumference26,659 m
  • Beam energy6.8 TeV (Run 3)
  • Bunches/beam2,808
  • Crossings/sec40 MHz
  • Luminosity2 × 10³⁴ cm⁻² s⁻¹
  • Magnets1,232 dipoles, 8.33 T

LHC Schematic

CMS ATLAS ALICE LHCb 26.7 km ring · 100 m underground
P. 07 / 18 — TIMELINE

A century of discovery.

1897 — J.J. Thomson

Cathode rays are particles ~2,000× lighter than the proton. The electron.

1911 — Rutherford

Gold-foil scattering: atoms have tiny dense nuclei.

1928 — Dirac

Relativistic equation for the electron predicts antimatter. Confirmed by Anderson's positron, 1932.

1933 — Pauli & Fermi

Neutrino postulated to save β-decay's energy budget. Detected 1956 by Cowan & Reines.

1947 — Powell

π-meson found in cosmic rays — Yukawa's predicted strong-force carrier.

1964 — Gell-Mann, Zweig

Quarks proposed to organize the hadron zoo. Confirmed by SLAC deep-inelastic scattering, 1968.

1973 — GIM & QCD

Glashow–Iliopoulos–Maiani; asymptotic freedom (Gross, Politzer, Wilczek — Nobel 2004).

1983 — UA1, UA2

W and Z bosons observed at CERN's SppS — Rubbia and van der Meer Nobel.

1995 — CDF, D0

Top quark confirmed at Fermilab — last quark of generation 3.

1998 — Super-Kamiokande

Atmospheric neutrino oscillations — neutrinos have mass.

2012 — ATLAS & CMS

Higgs boson, m = 125 GeV.

2023 — Muon g−2 (Fermilab)

Combined aμ tension with theory: 4.2σ. New physics or hadronic uncertainty?

P. 08 / 18
Detector visualization

Inside the detector.

Concentric layers — silicon trackers, electromagnetic and hadronic calorimeters, muon chambers. A single bunch crossing yields ~30 pile-up vertices; reconstruction software disentangles them in real time.

P. 09 / 18 — KEY FIGURES

Architects of the SM.

Marie Curie

1867–1934. Discovered radium, polonium; only person with Nobels in two sciences.

P. A. M. Dirac

1902–84. Relativistic QM, antimatter, magnetic monopoles. Famously laconic.

Richard Feynman

1918–88. QED, path integrals, diagrams, bongos. Nobel 1965.

Chien-Shiung Wu

1912–97. Co-found parity violation in β-decay, 1956.

Murray Gell-Mann

1929–2019. Strangeness, the Eightfold Way, quarks. Nobel 1969.

Edward Witten

b. 1951. M-theory unification, Fields Medal 1990.

Peter Higgs

1929–2024. Predicted scalar boson, 1964. Nobel 2013.

Fabiola Gianotti

b. 1960. ATLAS spokesperson during Higgs discovery; CERN DG since 2016.

Higgs_boson
P. 10 / 18 — NEUTRINOS

The ghost particles.

Neutral, almost massless, near-light-speed. Each second, ~6.5 × 10¹⁰ solar neutrinos cross every cm² of you. Almost all pass through unhindered.

They oscillate between flavors (e, μ, τ) — observed by SNO and Super-K, Nobel 2015. This requires nonzero mass; sums of mass eigenstates < 0.12 eV from cosmology.

|να⟩ = Σ Uαi |νi

Open: are they Majorana (their own antiparticles)? Is there CP violation in their mixing? Both could explain the cosmic matter–antimatter asymmetry.

Oscillation Probability

P(νμ→νμ) P(νμ→ντ) L/E

Sinusoidal flavor mixing

P. 11 / 18 — BEYOND THE STANDARD MODEL

Where the SM cracks.

Dark matter

5× more than baryonic matter. Not in the SM. Candidates: WIMPs, axions, sterile νs, primordial black holes, dark photons.

Neutrino masses

SM has them strictly massless. Seesaw mechanisms add right-handed Majorana νR at high scale.

Hierarchy problem

Why mH = 125 GeV ≪ MPl = 1.2 × 10¹⁹ GeV? Quantum corrections should push it up. SUSY? Compositeness?

Strong CP

QCD allows CP violation θ̄ ≤ 10⁻¹⁰. Why so small? Peccei–Quinn symmetry → axion.

Matter–antimatter asymmetry

Sakharov conditions: B-violation, C/CP-violation, departure from equilibrium. SM CP-violation insufficient.

Quantum gravity

No renormalizable QFT for spin-2 gravity. Strings. Loop quantum gravity. Asymptotic safety.

P. 12 / 18 — PULL QUOTE
"The first principle is that you must not fool yourself — and you are the easiest person to fool."
— RICHARD FEYNMAN, CALTECH 1974
P. 13 / 18 — SUPERSYMMETRY

SUSY & its discontents.

Supersymmetry posits a partner for every SM particle differing in spin by ½: squarks for quarks, sleptons for leptons, gauginos for gauge bosons. Elegantly cancels the quadratic divergences in the Higgs mass. Predicts a stable lightest supersymmetric particle — a natural dark matter candidate.

After 13 years of LHC data, no superpartners have been found below ~2 TeV. The minimal scenarios are excluded; less natural ones remain alive but bruised.

Particles & Sparticles

SMSUSY quark qsquark q̃ lepton ℓslepton ℓ̃ photon γphotino γ̃ gluon ggluino g̃ Higgs HHiggsino H̃
FIG. 3
Standard Model chart.
The Standard Model — the theory of fundamental particles. Includes 17 particles (with the Higgs); does not include gravity.
P. 14 / 18 — UNIFICATION

One force, many vibrations.

Three approaches knock heads against quantum gravity:

  • String theory10D, branes, dualities — Witten's M-theory unifies the 5 string types.
  • LQGSpin networks; spacetime as woven fabric.
  • Asymptotic safetyGravity has nontrivial UV fixed point; Weinberg's idea.

Coupling constants α1, α2, α3 nearly meet at ~10¹⁶ GeV under SUSY running — hint at a Grand Unified Theory.

Running Couplings

α₁ U(1) α₂ SU(2) α₃ SU(3) log(μ/GeV) ~10¹⁶ GeV
P. 15 / 18 — FRONTIER

What's next.

HL-LHC

2030 onwards. ×10 luminosity. Higgs self-coupling, rare decays, precision electroweak.

FCC

100 km tunnel under Geneva, e⁺e⁻ then 100 TeV pp. Decision pending; commissioning ~2045.

Muon collider

3–10 TeV in compact ring; muons radiate less synchrotron — but hard to cool. R&D underway.

DUNE / Hyper-K

Long-baseline neutrino oscillations; CP violation in lepton sector; proton decay.

LZ / XENONnT

Multi-tonne liquid xenon, kilometres deep. WIMP cross-sections under 10⁻⁴⁸ cm².

ADMX / haloscopes

Resonant cavities sweep μeV–meV axion masses. Could find dark matter this decade.

P. 16 / 18 — OPEN QUESTIONS

The uncomfortable ones.

P. 17 / 18 — GO DEEPER

Watch & read.

PBS Space Time — Particle Physics Series

Plus Veritasium "Why this Higgs result is so important" — and Fermilab's Don Lincoln channel for unfiltered detail.

Watch ↗

References

  • Peskin & SchroederIntro to QFT (1995)
  • WeinbergQFT vols I–III (1995)
  • GriffithsIntro to Elementary Particles
  • PDGReview of Particle Physics — open access
  • ATLAS & CMS2012 Higgs papers in Phys. Lett. B
  • WilczekThe Lightness of Being (2008)
P. 18 / 18 — END

END OF BLUEPRINT.

Drawing reviewed for accuracy as of 2026.05. Standard Model is provisional pending discovery of new physics at higher scales.