research
Physics of Neutron Star Crusts
- Authors
- A Bohr
- A Bulgac
- A Burrows
- A Cumming
- A Gelfert
- A Melatos
- A Schwenk
- A Sedrakian
- A Sedrakian
- A Spitkovsky
- A Zeilinger
- AA Abrikosov
- AB Migdal
- AD Kaminker
- AD Kaminker
- AD Kaminker
- AD Kaminker
- AD Sedrakian
- AD Sedrakian
- AF Andreev
- AG Lyne
- AG Lyne
- AI Chugunov
- AI Chugunov
- AK Dutta
- AL Fetter
- AL Piro
- AL Piro
- AL Piro
- AL Piro
- AL Watts
- AS Botvina
- AY Potekhin
- AY Potekhin
- B Abbott
- B Abbott
- B Carter
- B Carter
- B Carter
- B Carter
- B Carter
- B Carter
- B Carter
- B Carter
- B Carter
- B Carter
- B Carter
- B Carter
- B Carter
- B Carter
- B Carter
- B Carter
- B Haskell
- B Haskell
- B Hüttner
- B Jönsson
- B Link
- B Link
- B Link
- B Link
- BM Pontecorvo
- BM Pontecorvo
- C Barat
- C Cutler
- C Kittel
- C Monrozeau
- C Peralta
- C Peralta
- CJ Gorter
- CJ Horowitz
- CJ Jog
- CJ Pethick
- CJ Pethick
- CJ Pethick
- CL Inman
- CP Lorenz
- CP Lorenz
- D Chakrabarty
- D Harding
- D Legut
- D Page
- DA Kirszhnits
- DA Kirzhnits
- DG Ravenhall
- DG Ravenhall
- DG Yakovlev
- DG Yakovlev
- DG Yakovlev
- DG Yakovlev
- DG Yakovlev
- DJ Dean
- DK Galloway
- DR Tilley
- DS Tsakadze
- DZ Freedman
- E Chabanat
- E Chabanat
- E Chabanat
- E Flowers
- E Flowers
- E Flowers
- E Gourgoulhon
- E Khan
- E Vigezzi
- E Wigner
- EB Sonin
- EE Kolomeitseiv
- EF Brown
- EJ Yarmchuk
- EL Andronikashvili
- EM Cackett
- F Barranco
- F Barranco
- F Blasio de
- F Douchin
- F Douchin
- F Douchin
- F Douchin
- F Haberl
- F Hund
- F Hund
- F London
- F Montani
- FD Mackie
- FJ Dyson
- FV Blasio de
- FV Blasio de
- FV Blasio de
- FV Blasio de
- FV Blasio de
- FV Blasio de
- G Audi
- G Baym
- G Baym
- G Baym
- G Baym
- G Baym
- G Gori
- G Greenstein
- G Hobbs
- G Martínez-Pinedo
- G Mendell
- G Watanabe
- G Watanabe
- G Watanabe
- GA Williams
- GL Israel
- GM Gandelman
- GM Gandelman
- GS Bisnovatyi-Kogan
- H Grigorian
- H Horner
- H Schatz
- H Schatz
- H Shen
- H Shen
- H Sonoda
- H Sotani
- H-T Janka
- H-Y Chiu
- H-Y Chiu
- I Easson
- I Easson
- I Prigogine
- I Slaus
- IH Stairs
- IM Khalatnikov
- J Bardeen
- J Bardeen
- J Dechargé
- J Dobaczewski
- J Grindlay
- J Kohanoff
- J McKenna
- J Miralda-Escudé
- J Shaham
- J Ventura
- J-R Buchler
- JA Sauls
- JB Hartle
- JB Kinney
- JC Slater
- JD Gelfand
- JF Annett
- JJM Zand in’t
- JM Lattimer
- JM Lattimer
- JM Lattimer
- JM Lattimer
- JM Ziman
- JR Oppenheimer
- JR Stone
- JS Heyl
- JS Tsakadze
- JW Negele
- JW Negele
- JWT Hessels
- K Fuchs
- K Glampedakis
- K Glampedakis
- K Glampedakis
- K Iida
- K Iida
- K Iida
- K Langanke
- K Oyamatsu
- K Oyamatsu
- K Oyamatsu
- K Sato
- K Shimizu
- K Sumiyoshi
- K Sumiyoshi
- K Sumiyoshi
- KP Levenfish
- KS Cheng
- L Bildsten
- L Bildsten
- L Lindblom
- L Lindblom
- L Onsager
- L Samuelsson
- L Tisza
- L Villain
- LB Leinson
- LB Leinson
- LD Landau
- LD Landau
- LD Landau
- LD Landau
- LG Cao
- LJ Campbell
- LM Franco
- LP Gorkov
- M Alford
- M Arnould
- M Baldo
- M Baldo
- M Baldo
- M Baldo
- M Baldo
- M Bejger
- M Bender
- M Brack
- M Colpi
- M Farine
- M Hashimoto
- M Hirasawa
- M Lassaut
- M Matsuo
- M Matsuzaki
- M Morii
- M Motokowa
- M Onsi
- M Onsi
- M Prakash
- M Ruderman
- M Ruderman
- M Ruderman
- M Ruderman
- M Ruderman
- M Ruderman
- M Ruderman
- M Vavoulidis
- MA Alpar
- MA Alpar
- MA Alpar
- MA Alpar
- MA Alpar
- MB Larson
- ME Gusakov
- MY Fujimoto
- N Andersson
- N Andersson
- N Andersson
- N Andersson
- N Andersson
- N Andersson
- N Andersson
- N Bohr
- N Chamel
- N Chamel
- N Chamel
- N Chamel
- N Chamel
- N Chamel
- N Chamel
- N Itoh
- N Itoh
- N Itoh
- N Messios
- N Sandulescu
- N Sandulescu
- N Wang
- O Morsch
- O Penrose
- OL Caballero
- OY Gnedin
- P Avogadro
- P Bonche
- P Bonche
- P Donati
- P Donati
- P Donati
- P Gögelein
- P Haensel
- P Haensel
- P Haensel
- P Haensel
- P Haensel
- P Haensel
- P Haensel
- P Haensel
- P Jaikumar
- P Jaranowski
- P Kaaret
- P Magierski
- P Nozières
- P Ring
- PB Jones
- PB Jones
- PB Jones
- PB Jones
- PG Gennes de
- PG Gennes de
- PJ Feibelman
- PM Pizzochero
- PM Pizzochero
- PM Woods
- PN McDermott
- PS Shternin
- PS Shternin
- PS Shternin
- PW Anderson
- PW Anderson
- R Beig
- R Combescot
- R Giacconi
- R Nandkumar
- R Ogasawara
- R Prix
- R Prix
- R Ruderman
- R Smoluchowski
- RA Broglia
- RA Duine
- RA Wolf
- RC Duncan
- RC Tolman
- RE Packard
- RE Rutledge
- RI Epstein
- RI Epstein
- RP Feynman
- RP Feynman
- RP Feynman
- S Balibar
- S Bonazzola
- S Dall’Osso
- S Goriely
- S Goriely
- S Gupta
- S Heinz
- S Ogata
- SB Rüster
- SL Shapiro
- ST Belyaev
- T Ellis
- T Maruyama
- T Papenbrock
- T Strohmayer
- T Strohmayer
- T Wong
- TE Sterne
- TE Strohmayer
- TE Strohmayer
- TE Strohmayer
- TE Strohmayer
- TE Strohmayer
- TE Strohmayer
- TJ Bürvenich
- TV Shabanova
- U Geppert
- U Lee
- U Lombardo
- VI Ritus
- VI Ritus
- VK Tkachenko
- VK Tkachenko
- VL Ginzburg
- VL Ginzburg
- VL Ginzburg
- VM Kaspi
- VM Kaspi
- VM Kaspi
- VR Pandharipande
- VR Pandharipande
- W Hillebrandt
- W Ketterle
- W Kohn
- WF Vinen
- WG Newton
- Y Levin
- Y Levin
- Y Mochizuki
- Y Pomeau
- Y Yu
- YL Vartanyan
- Z Medin
- Ø Elgarøy
- Ø Elgarøy
- Ø Elgarøy
- Publication date
- 1 January 2008
- Publisher
- 'Living Reviews'
- Doi
Abstract
The physics of neutron star crusts is vast, involving many different research fields, from nuclear and condensed matter physics to general relativity. This review summarizes the progress, which has been achieved over the last few years, in modeling neutron star crusts, both at the microscopic and macroscopic levels. The confrontation of these theoretical models with observations is also briefly discussed.Comment: 182 pages, published version available at <http://www.livingreviews.org/lrr-2008-10Similar works
Available Versions
Last time updated on 04/06/2019
Last time updated on 28/04/2017