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Gamma-Ray Burst Science in 2030

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Palabras clave – provistas por la editorial

gamma rays bursts; radiation mechanisms; non-thermal; quark matter; up-down quark nuggets; quark star crusts; white dwarfs; gamma ray bursts; fireball model; circularity problem; standard candles; calibration; dark energy; dark matter; cosmography; cosmological parameters; Gamma-ray bursts; massive stars; supernova; spectroscopy; binary stars; metallicity; rotation rate; gamma-ray bursts; polarization; jet structure; instruments & methods; GRB; radio; redshift evolution; instrumentation—detectors; gamma rays: general; gamma-ray bursts: general; gamma-ray burst; gravitational wave; neutron stars; magnetosphere; shock breakout; SVOM (Space-based multiband astronomical Variable Objects Monitor); time-domain astronomy; γ-ray burst; multi-messenger astrophysics; nano-satellites; supernovae; Ia; cosmology; Hubble; tension; ΛCDM; evolution; modified; gravity; theories; prompt emission; relativistic jets; gamma–rays: bursts; cosmology: early universe; multi-messenger astrophysics: gravitational waves; neutrinos; instrumentation: X/gamma–ray astrophysics from space; fundamental physics; non-thermal processes; Cherenkov telescopes; very high energy; IACTs; clustering; statistical analysis; feature extraction; machine learning; gamma-ray burst: general; relativistic processes; magnetohydrodynamics

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