multi-messenger-astrophysics

Layer 1 — Physics24 concepts in this subtree

Multi-messenger astrophysics — the study of astrophysical events observed simultaneously through multiple cosmic messengers: electro-magnetic radiation (γ / X / UV / visible / IR / radio), gravitational waves, neutrinos, and…

Chirp mass: M_c = (m1·m2)^(3/5) / (m1+m2)^(1/5)
GW-EM delay: Δt = d·(1/v_gw - 1/c)
Inspiral frequency evolution: f(t) ∝ (t_c − t)^(-3/8)
Chirp-mass equal-mass: M_c(m_1=m_2=m) = 2^(4/5)·m/2
GW-EM simultaneity: Δt(v_gw=c) = 0
Inspiral-frequency ratio: f(t_c/2)/f(0) = 2^(3/8)
GW chirp mass M_chirp = (m_1 m_2)^{3/5}/(m_1+m_2)^{1/5}; Holder/Minkowski moments
Standard-siren Hubble: H_0 = c z/d_L (low-z limit); luminosity distance via metric
Multi-messenger achromaticity: Delta t = D(1/v_GW - 1/c) = 0 at v_GW = c (Hasse-Minkowski)
Theorem: M_chirp * 2^{1/5} - m = 0 at m_1 = m_2 = m (equal-mass chirp-mass identity)
Theorem: H_0 d_L - c z = 0 (standard-siren Hubble identity at low z)
Theorem: Delta t at v_GW = c equals 0 (GW170817 multi-messenger achromaticity)
Gravitational wave detection (LIGO 2015)
Neutrino astronomy (IceCube)
Kilonova GW170817 (binary neutron star)
UHECR detection (Pierre Auger)
Fast radio bursts (FRB)
Dark matter direct detection (XENON)
GW170817 (2017)
GW150914 (2015)
PTA nHz (NANOGrav 2023)
Kilonova (2017)
TXS 0506 (IceCube 2018)
Primordial GW (BICEP/Keck)
Explore the multi-messenger-astrophysics subtree on the interactive graph →