[1] L. W. Kebede, “Relativistic Plasma Diffusion: A Possible Source for Neutron Star Magnetic Field,” Astrophysics and Space Science, Vol. 282, No. 1, 2002, pp. 131-140.
[2] J. E. Rhoads, “The Dynamics and Light Curves of Beamed Gamma-Ray Burst Afterglows,” The Astrophysical Journal, Vol. 525, No. 2, 1999, pp. 737-749. http://dx.doi.org/10.1086/307907
[3] D. A. Frail, et al., “Beaming in Gamma-Ray Bursts: Evidence fir a Standard Energy Reservoir,” Astrophysical Journal, Vol. 562, No. 1, 2001, pp. L55-L58. http://dx.doi.org/10.1086/338119
[4] E. Berger, et al., “A Standard Kinetic Energy Reservoir in Gamma Ray Burst Afterglows,” Astrophysical Journal, Vol. 590, No. 1, 2003, pp. 379-385. http://dx.doi.org/10.1086/374892
[5] D. Bhattacharya, “The Evolution of the Magnetic Fields of Neutron Stars,” JApAs, Vol. 16, No. 2, 1995, pp. 217-232.
[6] E. Phinney and S. Kulkarni, “Binary and Millisecond Pulsars,” ARA. & A., Vol. 32, 1994, pp. 591-639.
[7] G. Baym, C. Pethick and D. Pines, “Spin Up in Neutron Stars: The Future of the Vela Pulsar,” Nature, Vol. 224, No. 5222, 1969, pp. 872-874. http://dx.doi.org/10.1038/224872a0
[8] V. Uprin and D. Yakovlev, “Thermogalvanomagnetic Effects in White Dwarfs and Neutron Stars,” Soviet Astronomy, Vol. 24, 1980, pp. 425-435.
[9] S. Yamada, K. Kotake and T. Yamasaki, “The Role of Neutrinos, Rotations and Magnetic Fields in Collapse-Driven Supernovae,” New Journal of Physics, Vol. 6, No. 1, 2004, pp. 79-102.
http://dx.doi.org/10.1088/1367-2630/6/1/079
[10] D. Lai and S. L. Shapiro, “Cold Equation of State in a Strong Magnetic Field—Effects of Inverse Beta-Decay,” Astrophysical Journal, Vol. 383, Pt. 1, 1991, pp. 745-751. http://dx.doi.org/10.1086/170831
[11] L. W. Kebede, “Neutron Star Magnetic Field Dynamics and Its Evolution,” MNRAS, Vol. 282, No. 3, 1996, pp. 845-852. http://dx.doi.org/10.1093/mnras/282.3.845
[12] D. Pines, “Pulsars and Compact X-Ray Sources—Cosmic Laboratories for the Study of Neutron Stars and Hadron Matter,” Journal de Physique, Vol. 41C2, No. 3, 1980, pp. C2-111-C2-124.
[13] P. Haensel, “Equations of State of Dense Matter and Maximum Mass of Neutron Stars,” EAS, Vol. 7, 2003, pp. 249-282.
[14] J. M. Lattimer and M. Parakash, “The Physics of Neutron Stars,” Science, Vol. 304, No. 5670, 2004, pp. 536-542. http://dx.doi.org/10.1126/science.1090720
[15] P. Haensel, “Apparent Radii of Neutron Stars and Equation of State of Dense Matter,” Astronomy and Astrophysics, Vol. 380, 2001, pp. 186-189
[16] F. Pacini, “Energy Emission from a Neutron Star,” Nature, Vol. 216, No. 5115, 1967, pp. 567-568. http://dx.doi.org/10.1038/216567a0
[17] F. Pacini, “Rotating Neutron Stars,” Nature, Vol. 219, No. 5150, 1968, pp. 145-146.
http://dx.doi.org/10.1038/219145a0
[18] J. E. Gunn and J. P. Ostriker, “Magnetic Dipole Radiation from Pulsars,” Nature, Vol. 221, No. 1, 1969, pp. 454-456. http://dx.doi.org/10.1038/221454a0
[19] D. Arnett and R. Bowers, “A Microscopic Interpretation of Neutron Star Structure,” Astrophysical Journal, Vol. 33, 1977, pp. 415-436.
[20] C. D. Ott, A. Burrows, T. A. Thompson, E. Livine and R. Walder, “The Spin Period and Positional Profiles of Neutron Stars at Birth,” The Astrophysical Journal Supplement, Vol. 164, No. 1, 2006, pp. 130-155. http://dx.doi.org/10.1086/500832
[21] S. Weinberg, “Gravitation and Cosmology: Principles and Applications of the General Theory of Relativity,” Wiley, New York, 1972.
[22] D. Lai, D. F. Chernoff and J. M. Cordes, “Pulsar Jets: Implications for Neutron Star Kicks and Initial Spins,” Astrophysical Journal, Vol. 549, 2001, pp. 1111-1118. http://dx.doi.org/10.1086/319455
[23] B. Paczynski, “Gamma-Ray Bursters at Cosmological Distances,” Astrophysical Journal, Vol. 308, Pt. 2, 1986, pp. L43-L46. http://dx.doi.org/10.1086/184740
[24] J. Goodman, “Are Gamma-Ray Bursts Optically Thick?” Astrophysical Journal, Vol. 308, Pt. 2, 1986, pp. L47-L50. http://dx.doi.org/10.1086/184741
[25] T. Piran, “Gamma-Ray Bursts and the Fire-Ball Model,” Physics Reports, Vol. 314, No. 6, 1999, pp. 575-667. http://dx.doi.org/10.1016/S0370-1573(98)00127-6
[26] G. Ghishellini, A. Celotti and D. Lazzati, “Constraints on the Emission Mechanisms of Gamma-Ray Bursts,” MNRAS, Vol. 313, No. 1, 2000, pp. L1-L5. http://dx.doi.org/10.1046/j.1365-8711.2000. 03354.x
[27] V. V. Usov, “Millisecond Pulsars with Extremely Strong Magnetic Fields as a Cosmological Source of Gamma-Ray Bursts,” Nature, Vol. 357, No. 6378, 1992, pp. 472-474. http://dx.doi.org/10.1038/ 357472a0
[28] M. Lyutikov and R. Blandford, “Gamma-Ray Bursts as Electromagnetic Outflows,” arXiv:astro-ph/0312347v1, 2003, 78p.
[29] J. C. Wheeler, I. Yi, P. Hoflich and L. Wang, “Asymmetric Supernova, Pulsars, Magnetars, and Gamma-Ray Bursts,” Astrophysical Journal, Vol. 537, No. 2, 2000, pp. 810-823. http://dx.doi.org/10. 1086/309055
[30] T. A. Thompson, P. Chang and E. Quataert, “Magnetar Spin Down, Hyperenergetic Supernovae, and Gamma Ray Bursts,” Astrophysical Journal, Vol. 611, No. 1, 2004, pp. 380-393. http://dx.doi.org/ 10.1086/421969
[31] B. D. Metzger, T. A. Thompson and E. Quataert, “Proto-Neutron Star Winds with Magnetic Fields and Rotation,” Astrophysical Journal, Vol. 659, 2007, pp. 561-579. http://dx.doi.org/10.1086/512059
[32] N. Lyons, P. O’Brien, B. Zhang, R. Willingale, E. Troja and R. Starling, “Can X-Ray Emission Powered by a Spinning-Down Magnetar Explain Some Gamma-Ray Burst Light-Curve Features?” MNRAS, Vol. 402, No. 2, 2010, pp. 705-712. http://dx.doi.org/10.1111/j.1365-2966.2009.15538.x
[33] E. Troja, G. Cusumano, P. O’Brien, B. Zhang, B. Sbarufatti, V. Mangano, R. Willingale, G. Chincarini, J. Osborne, F. Marshall, et al., “Swift Observations of GRB070110: An Extra X-Ray Afterglow powered by the Central Engine,” Astrophysical Journal, Vol. 665, No. 1, 2007, pp. 599-607. http://dx.doi.org/ 10.1086/519450
[34] D. Bhattacharya, R. Wijers, J. Hartman and F. Verbent, “On the Decay of the Magnetic Field of Single Radio Pulsars,” Astronomy and Astrophysics, Vol. 254, 1992, pp. 198-212.
[35] S. Konar and D. Bhattacharya, “Magnetic Field Evolution of Accreting Neutron Stars-II,” MNRAS, Vol. 303, No. 3, 1999, pp. 588-594. http://dx.doi.org/10.1046/j.1365-8711.1999.02287.x
[36] V. M. Kaspi and M. A. McLaughlin, “Chandra X-Ray Detection of the High Magnetic Field Radio Pulsar, PSR J1718-3718,” Astrophysical Journal, Vol. 618, No. 1, 2005, pp. L41-L44. http://dx.doi.org/10. 1086/427628
[37] M. Gonzalez, V. Kaspi, A. Lyne and M. Pivovaroff, “An XMM-Newton Observation of the High Magnetic Field Radio Pulsar, PSR B0154+61,” Astrophysical Journal, Vol. 610, No. 1, 2004, pp. L37-L40. http://dx.doi.org/10.1086/423033
[38] J. R. Lin and S. N. Zhang, “Radio Pulsars are Progenitors of Anomalous X-Ray Pulsars and Soft Gamma-Ray Repeaters: Magnetic Field Evolution through Pulsar Glitches,” Astrophysical Journal, Vol. 615, No. 2, 2004, pp. L133-L136. http://dx.doi.org/10.1086/426316
[39] M. Lyutikov, “Explosive Reconnection in Magnetars,” MNRAS, Vol. 346, No. 2, 2003, pp. 540-554. http://dx.doi.org/10.1046/j.1365-2966.2003.07110.x
[40] M. J. Aschwanden, A. I. Poland and D. M. Rabin, “The New Solar Corona,” Astronomy and Astrophysics, Vol. 39, 2001, pp. 175-210. http://dx.doi.org/10.1146/annurev.astro.39.1.175