Irodov Problem 6.286 — Resonances — Delta Baryon

Problem Statement

Problem Statement

The $\Delta^{++}$ resonance appears in $\pi^+ + p$ scattering at $E_{CM} = 1232\,\text{MeV}$. The width is $\Gamma = 120\,\text{MeV}$. Find the mean lifetime of the $\Delta^{++}$.

Given Information

• $\Gamma = 120\,\text{MeV}$ (resonance width), $E_{CM} = 1232\,\text{MeV}$ (rest mass)

Physical Concepts & Formulas

By the time-energy uncertainty principle, a resonance of width $\Gamma$ has lifetime $\tau = \hbar/\Gamma$. The $\Delta(1232)$ is a $uuu$ (for $\Delta^{++}$) baryon with $J^P = 3/2^+$, decaying strongly via $\Delta \to N + \pi$. Its width $\Gamma = 120\,\text{MeV}$ gives an extremely short strong-interaction lifetime.

• $\tau = \hbar/\Gamma$; $\hbar = 6.582\times10^{-25}\,\text{GeV·s}$

Step-by-Step Solution

$$\tau = \frac{\hbar}{\Gamma} = \frac{6.582\times10^{-25}\,\text{GeV·s}}{0.120\,\text{GeV}} = 5.49\times10^{-24}\,\text{s}$$

Worked Calculation

$$\tau = \frac{\hbar c}{\Gamma c} = \frac{197.3\,\text{MeV·fm}}{120\,\text{MeV} \times 3\times10^{23}\,\text{fm/s}} = \frac{197.3}{3.6\times10^{25}}\,\text{s} = 5.5\times10^{-24}\,\text{s}$$

Answer

$$\boxed{\tau = \hbar/\Gamma \approx 5.5\times10^{-24}\,\text{s}}$$

Physical Interpretation

The $\Delta(1232)$ lifetime of $5.5\times10^{-24}$ s is characteristic of strong interaction decay — about the time light takes to cross a proton ($R_p/c \sim 10^{-23}$ s). Resonances this short-lived cannot be detected directly; they appear as peaks in the energy-dependent cross-section (Breit-Wigner resonance). The $\Delta(1232)$ plays crucial roles in pion-nucleon interactions, nuclear structure, and astrophysics (delta isobar excitation in neutron stars).

Given Information

• $\hbar c = 197.3\,\text{MeV·fm}$; $\hbar = 6.582\times10^{-25}\,\text{GeV·s}$
• $\alpha_{EM} = 1/137.036$; $G_F/(\hbar c)^3 = 1.166\times10^{-5}\,\text{GeV}^{-2}$
• $m_p c^2 = 938.3\,\text{MeV}$; $m_\pi c^2 = 135\,\text{MeV}$ (neutral), $140\,\text{MeV}$ (charged)
• $m_\mu c^2 = 105.7\,\text{MeV}$; $m_W = 80.4\,\text{GeV}/c^2$; $m_Z = 91.2\,\text{GeV}/c^2$; $m_H = 125.1\,\text{GeV}/c^2$

Physical Concepts & Formulas

Elementary particle physics is governed by the Standard Model — a quantum field theory based on gauge symmetry $SU(3)_C \times SU(2)_L \times U(1)_Y$. Conservation laws (baryon number, lepton number, strangeness in strong interactions, energy-momentum, charge) determine which processes are allowed. Kinematics of relativistic reactions uses the Lorentz-invariant Mandelstam variables $s, t, u$; the threshold condition requires $\sqrt{s} = \sum m_{final} c^2$ at minimum.

• $s = (p_1 + p_2)^2 c^2 = E_{CM}^2$ — Mandelstam $s$ (squared CM energy)
• $T_{th} = [(\sum m_f)^2 – (\sum m_i)^2]c^4/(2m_{target}c^2)$ — threshold kinetic energy
• $\tau = \hbar/\Gamma$ — particle lifetime from decay width
• $P(\nu_\alpha \to \nu_\beta) = \sin^2(2\theta)\sin^2(1.27\Delta m^2 L/E)$ — neutrino oscillation probability

Step-by-Step Solution

Step 1 — Apply 4-momentum conservation: In any particle reaction, total 4-momentum is conserved. Compute the invariant mass $\sqrt{s}$ of the initial state and match to the final state mass sum at threshold.

$$\sqrt{s} = \sqrt{(E_1+E_2)^2/c^2 – (\mathbf{p}_1+\mathbf{p}_2)^2} = \sum_{final} m_i c^2 \quad (\text{at threshold})$$

Step 2 — Check all conservation laws: Baryon number $B$, lepton numbers $L_e, L_\mu, L_\tau$, charge $Q$, strangeness $S$ (strong/EM only), isospin $I$ (strong only).

Step 3 — Calculate observable quantities: Masses, lifetimes ($\tau = \hbar/\Gamma$), branching ratios, oscillation lengths, cross-sections.

Worked Calculation

Applying the threshold formula or Breit-Wigner resonance formula to the given particle masses and widths, using the conversion $\hbar = 6.582\times10^{-25}\,\text{GeV·s}$ for lifetime calculations and $\hbar c = 197.3\,\text{MeV·fm}$ for cross-section estimates.

Answer

$$\boxed{\text{See derivation above for specific numerical results}}$$

Physical Interpretation

The Standard Model has been tested to extraordinary precision across 17 orders of magnitude in energy, from atomic physics to LHC collisions at 13 TeV. Despite this success, it cannot be the final theory: it does not include gravity, dark matter, dark energy, or a mechanism for the observed matter-antimatter asymmetry. Neutrino masses (discovered via oscillations) require SM extensions. The hierarchy problem (why $m_H \ll m_{Planck}$) motivates supersymmetry, extra dimensions, or compositeness. The next generation of experiments (HL-LHC, DUNE, CMB-S4, gravitational wave observatories) aims to discover the physics that lies beyond.