neutron star basics
A solar mass consists of ~ 1057 nucleons. If they are separated by typical inter-nucleon distances, what would the radius of the volume containing them be?
neutron star basics A solar mass consists of ~ 10 57 nucleons. If - - PowerPoint PPT Presentation
neutron star basics A solar mass consists of ~ 10 57 nucleons. If they are separated by typical inter-nucleon distances, what would the radius of the volume containing them be? neutron star basics
A solar mass consists of ~ 1057 nucleons. If they are separated by typical inter-nucleon distances, what would the radius of the volume containing them be?
∼ ·
λ
E A ≈ −aV + aSA−1/3 + aA N − Z N + Z ⇥2 + aC Z2 A4/3
see review by Lattimer & Prakash
= . − = /( + ), = = . ε(, ) = ε() + ε()( − ).
β µ = µ − µ = ∂ε ∂
∂ε ∂
−∂ε ∂ = ε( − ). µ = (π)/, =
≈ . ε =
µe kT, mec2 Z2e2 a kT
µe kT, mec2 Z2e2 a kT
µe kT, mec2 Z2e2 a kT
➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ ➤ O (8) F (9) Ne (10) Na (11) Mg (12) Al (13) Si (14) P (15) S (16) Cl (17) Ar (18) K (19) Ca (20) Sc (21) Ti (22) V (23) Cr (24) Mn (25) Fe (26) Co (27) Ni (28)
S n (MeV) 9 18
8 10 12 14 16 18 20 22 24 26 28 30 32 34 36 38 40 42 44 46 48
Z ↑
Sato ’79; Haensel & Zdunk ’90; Gupta et al. ’07; Steiner ’12; Schatz et al. ‘13; Lau et
illustration with a simple liquid-drop model (Mackie & Baym ’77, following Haensel & Zdunik ’90) pycnonuclear reactions neutron drip
Disordered nuclear pasta, magnetic field decay, and crust cooling in neutron stars
1Department of Physics and Center for the Exploration of Energy and Matter,
Indiana University, Bloomington, IN 47405, USA
2University Information Technology Services, Indiana University, Bloomington, IN 47408, USA 3Department of Physics, McGill University, 3600 rue University, Montreal QC, H3A 2T8 Canada
(Dated: October 9, 2014)