1 Astrophysical Constraints on Dense Matter in Neutron Stars
43
71. W. Del Pozzo, T.G.F. Li, M. Agathos, C. Van Den Broeck, S. Vitale, Demonstrating the
feasibility of probing the neutron-star equation of state with second-generation gravitationalwave detectors. Phys. Rev. Lett. 111(7), 071101 (2013). https://doi.org/10.1103/PhysRevLett.
111.071101
72. P.B. Demorest, T. Pennucci, S.M. Ransom, M.S.E. Roberts, J.W.T. Hessels, A two-solar-mass
neutron star measured using Shapiro delay. Nature 467, 1081–1083 (2010). https://doi.org/10.
1038/nature09466
73. D.D. Doneva, E. Gaertig, K.D. Kokkotas, C. Krüger, Gravitational wave asteroseismology of
fast rotating neutron stars with realistic equations of state. Phys. Rev. D: Part. Fields 88(4),
044052 (2013). https://doi.org/10.1103/PhysRevD.88.044052
74. J.M. Dong, U. Lombardo, W. Zuo, 3 PF 2 pairing in high-density neutron matter. Phys. Rev. C
87(6), 062801 (2013). https://doi.org/10.1103/PhysRevC.87.062801
75. T. Ebisuzaki, D. Sugimoto, T. Hanawa, Are X-ray bursts really of super-Eddington luminosities? Pub. Astr. Soc. Jap. 36, 551–566 (1984)
76. K.G. Elshamouty, C.O. Heinke, G.R. Sivakoff, W.C.G. Ho, P.S. Shternin, D.G. Yakovlev,
D.J. Patnaude, L. David, Measuring the cooling of the neutron star in cassiopeia a with all
chandra X-ray observatory detectors. Astrophys. J. 777, 22 (2013). https://doi.org/10.1088/
0004-637X/777/1/22
77. E. Farhi, R.L. Jaffe, Strange matter. Phys. Rev. D 30, 2379–2390 (1984). https://doi.org/10.
1103/PhysRevD.30.2379
78. M. Feroci et al.: The large observatory for X-ray timing (LOFT). Exp. Astron. 34, 415–444
(2012). https://doi.org/10.1007/s10686-011-9237-2
79. V. Ferrari, L. Gualtieri, A. Maselli, Tidal interaction in compact binaries: a post-Newtonian
affine framework. Phys. Rev. D: Part. Fields 85(4), 044045 (2012). https://doi.org/10.1103/
PhysRevD.85.044045
80. F. Foucart, L. Buchman, M.D. Duez, M. Grudich, L.E. Kidder, I. MacDonald, A. Mroue,
H.P. Pfeiffer, M.A. Scheel, B. Szilagyi, First direct comparison of nondisrupting neutron starblack hole and binary black hole merger simulations. Phys. Rev. D: Part. Fields 88(6), 064017
(2013). https://doi.org/10.1103/PhysRevD.88.064017
81. J. Frank, A. King, D.J. Raine, Accretion Power in Astrophysics, 3rd edn. (Cambridge
University Press, Cambridge, 2002)
82. P.C.C. Freire, Eccentric binary millisecond pulsars. ArXiv e-prints (2009)
83. P.C.C. Freire, N. Wex, The orthometric parametrization of the Shapiro delay and an improved
test of general relativity with binary pulsars. Mon. Not. R. Astron. Soc. 409, 199–212 (2010).
https://doi.org/10.1111/j.1365-2966.2010.17319.x
84. J.L. Friedman, S.M. Morsink, Axial instability of rotating relativistic stars. Astrophys. J. 502,
714 (1998). https://doi.org/10.1086/305920
85. B.A. Fryxell, S.E. Woosley, Finite propagation time in multidimensional thermonuclear
runaways. Astrophys. J. 261, 332–336 (1982). https://doi.org/10.1086/160344
86. I. Fushiki, D.Q. Lamb, New insights from a global view of X-ray bursts. Astrophys. J. 323,
L55–L60 (1987). https://doi.org/10.1086/185056
87. D.K. Galloway, N. Lampe, On the consistency of neutron-star radius measurements from
thermonuclear bursts. Astrophys. J. 747, 75 (2012). https://doi.org/10.1088/0004-637X/747/
1/75
88. D.K. Galloway, J. Lin, D. Chakrabarty, J.M. Hartman, Discovery of a 552 Hz burst oscillation
in the low-mass X-ray binary EXO 0748-676. Astrophys. J. 711, L148–L151 (2010). https://
doi.org/10.1088/2041-8205/711/2/L148
89. F. García, G. Zhang, M. Méndez, The cooling phase of Type I X-ray bursts observed with
RXTE in 4U 1820-30 does not follow the canonical F ∝ T 4 relation. Mon. Not. R. Astron.
Soc. 429, 3266–3271 (2013). https://doi.org/10.1093/mnras/sts583
90. K.C. Gendreau, Z. Arzoumanian, T. Okajima, The neutron star interior composition exploreR
(NICER): an explorer mission of opportunity for soft x-ray timing spectroscopy, in Society of
Photo-Optical Instrumentation Engineers (SPIE) Conference Series, vol. 8443 (2012) https://
doi.org/10.1117/12.926396
43
71. W. Del Pozzo, T.G.F. Li, M. Agathos, C. Van Den Broeck, S. Vitale, Demonstrating the
feasibility of probing the neutron-star equation of state with second-generation gravitationalwave detectors. Phys. Rev. Lett. 111(7), 071101 (2013). https://doi.org/10.1103/PhysRevLett.
111.071101
72. P.B. Demorest, T. Pennucci, S.M. Ransom, M.S.E. Roberts, J.W.T. Hessels, A two-solar-mass
neutron star measured using Shapiro delay. Nature 467, 1081–1083 (2010). https://doi.org/10.
1038/nature09466
73. D.D. Doneva, E. Gaertig, K.D. Kokkotas, C. Krüger, Gravitational wave asteroseismology of
fast rotating neutron stars with realistic equations of state. Phys. Rev. D: Part. Fields 88(4),
044052 (2013). https://doi.org/10.1103/PhysRevD.88.044052
74. J.M. Dong, U. Lombardo, W. Zuo, 3 PF 2 pairing in high-density neutron matter. Phys. Rev. C
87(6), 062801 (2013). https://doi.org/10.1103/PhysRevC.87.062801
75. T. Ebisuzaki, D. Sugimoto, T. Hanawa, Are X-ray bursts really of super-Eddington luminosities? Pub. Astr. Soc. Jap. 36, 551–566 (1984)
76. K.G. Elshamouty, C.O. Heinke, G.R. Sivakoff, W.C.G. Ho, P.S. Shternin, D.G. Yakovlev,
D.J. Patnaude, L. David, Measuring the cooling of the neutron star in cassiopeia a with all
chandra X-ray observatory detectors. Astrophys. J. 777, 22 (2013). https://doi.org/10.1088/
0004-637X/777/1/22
77. E. Farhi, R.L. Jaffe, Strange matter. Phys. Rev. D 30, 2379–2390 (1984). https://doi.org/10.
1103/PhysRevD.30.2379
78. M. Feroci et al.: The large observatory for X-ray timing (LOFT). Exp. Astron. 34, 415–444
(2012). https://doi.org/10.1007/s10686-011-9237-2
79. V. Ferrari, L. Gualtieri, A. Maselli, Tidal interaction in compact binaries: a post-Newtonian
affine framework. Phys. Rev. D: Part. Fields 85(4), 044045 (2012). https://doi.org/10.1103/
PhysRevD.85.044045
80. F. Foucart, L. Buchman, M.D. Duez, M. Grudich, L.E. Kidder, I. MacDonald, A. Mroue,
H.P. Pfeiffer, M.A. Scheel, B. Szilagyi, First direct comparison of nondisrupting neutron starblack hole and binary black hole merger simulations. Phys. Rev. D: Part. Fields 88(6), 064017
(2013). https://doi.org/10.1103/PhysRevD.88.064017
81. J. Frank, A. King, D.J. Raine, Accretion Power in Astrophysics, 3rd edn. (Cambridge
University Press, Cambridge, 2002)
82. P.C.C. Freire, Eccentric binary millisecond pulsars. ArXiv e-prints (2009)
83. P.C.C. Freire, N. Wex, The orthometric parametrization of the Shapiro delay and an improved
test of general relativity with binary pulsars. Mon. Not. R. Astron. Soc. 409, 199–212 (2010).
https://doi.org/10.1111/j.1365-2966.2010.17319.x
84. J.L. Friedman, S.M. Morsink, Axial instability of rotating relativistic stars. Astrophys. J. 502,
714 (1998). https://doi.org/10.1086/305920
85. B.A. Fryxell, S.E. Woosley, Finite propagation time in multidimensional thermonuclear
runaways. Astrophys. J. 261, 332–336 (1982). https://doi.org/10.1086/160344
86. I. Fushiki, D.Q. Lamb, New insights from a global view of X-ray bursts. Astrophys. J. 323,
L55–L60 (1987). https://doi.org/10.1086/185056
87. D.K. Galloway, N. Lampe, On the consistency of neutron-star radius measurements from
thermonuclear bursts. Astrophys. J. 747, 75 (2012). https://doi.org/10.1088/0004-637X/747/
1/75
88. D.K. Galloway, J. Lin, D. Chakrabarty, J.M. Hartman, Discovery of a 552 Hz burst oscillation
in the low-mass X-ray binary EXO 0748-676. Astrophys. J. 711, L148–L151 (2010). https://
doi.org/10.1088/2041-8205/711/2/L148
89. F. García, G. Zhang, M. Méndez, The cooling phase of Type I X-ray bursts observed with
RXTE in 4U 1820-30 does not follow the canonical F ∝ T 4 relation. Mon. Not. R. Astron.
Soc. 429, 3266–3271 (2013). https://doi.org/10.1093/mnras/sts583
90. K.C. Gendreau, Z. Arzoumanian, T. Okajima, The neutron star interior composition exploreR
(NICER): an explorer mission of opportunity for soft x-ray timing spectroscopy, in Society of
Photo-Optical Instrumentation Engineers (SPIE) Conference Series, vol. 8443 (2012) https://
doi.org/10.1117/12.926396