Fields: Cosmology, Computational Astrophysics, Computer Science, Algorithms
Simulation post-processing tracks bound substructures across snapshots, assigning parent–child merge events with heuristic linking rules and uncertainty when disruptive tidal stripping fragments ident...
Fields: Astrophysics, Applied Mathematics
Linear adiabatic oscillation equations yield eigenvalue problems for pressure modes (p-modes) whose eigenfrequencies densely sample interior sound-speed profiles c(r) — analogous to recovering q(x) in...
Fields: Astrophysics, High Energy Astrophysics, Fluid Dynamics, Relativity
GRBs involve collimated flows with Lorentz factors inferred from opacity arguments and afterglow onset times. Internal shocks and external forward shocks convert kinetic energy into non-thermal partic...
Fields: Nuclear Physics, Astrophysics, Dense Matter, Qcd
Neutron stars support masses up to about two solar masses, constraining pressure versus density relations for matter above nuclear saturation. Microscopic models combine nucleonic matter, hyperons, or...
Fields: Astronomy, Astrophysics, Galaxy Formation, Stellar Populations
Star-forming galaxies occupy a blue cloud in color–magnitude space; quenched galaxies fall on a redder locus (the red sequence) with comparatively small scatter. The tightness implies synchronized ces...
Fields: Astronomy, Statistical Physics, Thermodynamics, Astrophysics
In normal thermodynamic systems, heat capacity C = dE/dT > 0: adding energy increases temperature. Lynden-Bell & Wood (1968, MNRAS 138:495) showed that self-gravitating systems have C < 0 — a fundamen...
Fields: Astrophysics, Star Formation, Cosmology
Giant molecular clouds are routinely characterized via virial estimates linking internal velocity dispersion σ and radius R to mass M ~ k σ² R / G when approximate equilibrium holds; galaxy clusters l...
Fields: Astrophysics, Chemistry, Nuclear Physics
The Burbidge, Burbidge, Fowler & Hoyle (B²FH, 1957) paper established that stellar nucleosynthesis accounts for the cosmic abundance of all elements: pp-chain and CNO cycle produce helium in main-sequ...
Fields: Astrophysics, Fluid Dynamics, Magnetohydrodynamics, Plasma Physics
Accretion disks around compact objects (black holes, neutron stars, white dwarfs, young stellar objects) must transport angular momentum outward to allow mass to flow inward. Molecular viscosity is 13...
Fields: Astrophysics, Plasma Physics, Fluid Mechanics
Solar wind turbulence is described by MHD as counter-propagating Alfvén wave packets interacting to drive a spectral energy cascade: outward-propagating Elsässer variables z+ (dominant) and inward-pro...
Fields: Astrophysics, Information Theory, Quantum Gravity, Theoretical Physics
The discovery that black holes have entropy proportional to their surface area — not volume — is the most profound known connection between spacetime geometry and information theory. 1. Bekenstein-Haw...
Fields: Astrophysics, Mathematics
Einstein's field equations Gμν + Λgμν = (8πG/c⁴)Tμν express that the curvature of spacetime (Einstein tensor Gμν, derived from the Riemann curvature tensor Rμναβ) equals the stress-energy content of m...
Fields: Astrophysics, Mathematics, Optics
The lensing map from source plane to image plane is a smooth map between two-dimensional planes, and its singularities form the critical curves in the image plane and caustic curves in the source plan...
Fields: Astrophysics, Nuclear Physics, Network Science
The abundance evolution of nuclides in a stellar burning zone is governed by a coupled ODE network dY_i/dt = sum_j lambda_{ji} Y_j - Y_i sum_k lambda_{ik}, where Y_i are molar abundances and lambda ar...
Fields: Astrophysics, Nuclear Physics, Physics
The neutron star mass-radius curve M(R) is a one-to-one map from the equation of state P(rho), determined by integrating the Tolman-Oppenheimer-Volkoff (TOV) equations; NICER X-ray timing measurements...
Fields: Astrophysics, Nuclear Physics, Particle Physics, Gravitational Wave Astronomy, Condensed Matter Physics
NEUTRON STAR INTERIOR PHYSICS: Nuclear saturation density: ρ₀ = 2.3×10¹⁴ g/cm³. Neutron star core: ρ = 2-8ρ₀ — accessible to no terrestrial experiment but observable via neutron star structure. TOLMAN...
Fields: Cosmology, Nuclear Physics, Astrophysics
Big Bang nucleosynthesis (BBN) traces abundances X_i(t) of ~26 nuclides from T~10 MeV (t~10⁻² s) to T~0.01 MeV (t~10³ s) using a coupled ODE system: dX_i/dt = Σ_j (production rates) - Σ_j (destruction...
Fields: Physics, Chemistry, Astrophysics
Neutron star interiors contain nuclear matter at densities exceeding nuclear saturation density (2×10^17 kg/m³); the equation of state is described by Landau Fermi liquid theory with strong nuclear in...
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