astroparticle-physics

Layer 1 — Physics24 concepts in this subtree

Interface of high-energy particle physics with cosmology and astrophysics: ultra-high-energy cosmic rays, extensive air showers, astrophysical neutrinos (IceCube), gamma-ray astronomy (HESS, CTA, Fermi-LAT), dark-matter direct detection…

Cosmic-ray primary spectrum: dN/dE ∝ E^{−2.7} below knee, E^{−3.0} above
GZK cutoff: E_th = (m_Δ² − m_p²)/(4·E_CMB) ≈ 5·10¹⁹ eV via p + γ_CMB → Δ⁺ → pπ⁰
Heitler EAS toy: N_max = E₀/E_c, X_max = X₀·log₂(E₀/E_c) for EM cascade
Neutrino astronomy (IceCube): diffuse astrophysical νₑ,ν_μ,ν_τ at TeV-PeV
Dark-matter direct detection: WIMP nuclear recoil, rate R ∝ ρ_χ·σ·⟨v⟩/m_χ
Axion haloscope: resonant cavity → microwave photon via B·a coupling
Fermi 2nd-order + 1st-order DSA: power-law spectrum from diffusion-advection FP
Liouville: cosmic-ray phase-space density f(x,p) conserved along trajectories
Blandford-McKee GRB fireball: self-similar Γ²(R) ~ E/(ρc²R^(3-k)) blast wave
Fermi DSA: s = 1 - log(P_esc)/log(β_ratio); s=2 for strong r=4 shock
Liouville: Jacobian det(∂(q,p)/∂(q₀,p₀))=1 for SHO Hamiltonian flow; df/dt=0
Blandford-McKee: Γ²(R) = 17E/(8πρc²R³); R_dec ~ E^(1/3); Γ²(2R)/Γ²(R) = 1/8
DM rotation curves (Rubin 1978)
Bullet cluster (Clowe 2006)
CMB Planck 2018 cosmological parameters
Primordial GW (LiteBIRD prospects)
Axion haloscope (Sikivie 1983)
Inflation (Guth 1981 / Linde-Albrecht-Steinhardt 1982)
Hess (1912)
GZK cutoff (1966)
Auger shower (1938)
IceCube (2013)
Direct DM (Goodman-Witten 1985)
Fermi-LAT (2018)
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