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Relevant bibliographies by topics / Magnetic field – pulsars

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Academic literature on the topic 'Magnetic field – pulsars'

Author: Grafiati

Published: 20 February 2023

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Journal articles on the topic "Magnetic field – pulsars"

1

Itoh, Naoki, and Takemi Kotouda. "Velocity-Magnetic Field Correlation of Pulsars." International Astronomical Union Colloquium 160 (1996): 49–50. http://dx.doi.org/10.1017/s0252921100040999.

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Monte Carlo simulations of the evolution of pulsars are carried out in order to compare with the recent measurement of the pulsar transverse velocity by Lyne &amp; Lorimer (1994). The new electron density distribution model of Taylor &amp; Cordes (1993) is adopted in the simulation. Accurate pulsar orbits in the Galactic gravitational field are calculated. It is found that the constant magnetic field model of pulsars can account for the new measurement of the pulsar transverse velocity and the apparent correlation between the strength of the magnetic field and the transverse velocity o

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Camilo, F. "Pulsar Period and Magnetic Field Evolution." International Astronomical Union Colloquium 160 (1996): 39–46. http://dx.doi.org/10.1017/s0252921100040975.

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AbstractOne of the important unsolved problems in pulsar astrophysics concerns the formation and evolution of their magnetic fields. We summarize measurements of braking indices and their implications for the spin and magnetic field evolution of young pulsars. An analysis of the period-period derivative diagram suggests one or more of the following: (a) a substantial population of young pulsars remains undiscovered; (b) a large fraction of all slow pulsars may be recycled; (c) magnetic fields in isolated pulsars decay by a factor of a few in the first few million years. We also note that the o

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Michel, F. Curtis. "Statistical Search for Magnetic Field Decay." International Astronomical Union Colloquium 128 (1992): 35–38. http://dx.doi.org/10.1017/s000273160015471x.

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AbstractThe claims made in many statistical analyses for magnetic field decay follow from the assumption that radio luminosity declines slower than spin-down luminosity which is suggested by least-squares fits to the data. However, such fits are very sensitive to the behaviors of the fastest and slowest pulsars. If pulsar luminosities are plotted in distance-selected groups, the (radio inefficient) Crab and Vela pulsars are clearly exceptional members and the remaining pulsars are consistent with a mean fixed conversion efficiency of 10–5. Numerical simulations (and theoretical analysis) stron

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COELHO, J. G., and M. MALHEIRO. "SIMILARITIES OF SGRs WITH LOW MAGNETIC FIELD AND WHITE DWARF PULSARS." International Journal of Modern Physics: Conference Series 18 (January 2012): 96–100. http://dx.doi.org/10.1142/s2010194512008276.

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Some of the most interesting types of astrophysical objects that have been intensively studied in the recent years are the Anomalous X-ray Pulsars (AXPs) and Soft Gamma-ray Repeaters (SGRs) seen usually as neutron stars pulsars with super strong magnetic fields. However, in the last two years two SGRs with low magnetic fields have been detected. Moreover, fast and very magnetic white dwarf pulsars have also been observed in the last years. Based on these new pulsar discoveries, white dwarf pulsars have been proposed as an alternative explanation to the observational features of SGRs and AXPs.

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Shibata, Shinpei. "Pulsar Electrodynamics — Pulsars and Puzzlers —." International Astronomical Union Colloquium 160 (1996): 409–16. http://dx.doi.org/10.1017/s0252921100041981.

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AbstractA gedanken experiment presented here provides basic understanding of how the pulsar magnetosphere operates. We discuss current issues about the electric-field acceleration along magnetic field lines and subsequent pair creation, and also about the pulsar wind problem. It is stressed that any local model, such as the inner gap model, the outer gap model and the pulsar wind model, must have free parameters to link it to other part of the magnetosphere.

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Lyne, A. G. "From Crab Pulsar to Magnetar?" Symposium - International Astronomical Union 218 (2004): 257–60. http://dx.doi.org/10.1017/s0074180900181100.

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We review the evolution of the Crab pulsar's rotational history during the past 35 years. Representing 3.7% of the pulsar's age, it is possible to estimate the likely development of the magnetic field and characteristic age much better than previously. The increasing magnetic field of this pulsar and of other young pulsars, most dramatically the Vela pulsar, raises the interesting possibility that these objects might evolve into magnetars. We discuss the observational case for such a proposal, but note that the origin of these field enhancements may be associated with glitch activity. However,

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Zhang, Jianwei, Chengmin Zhang, Di Li, et al. "Revisiting the Magnetic Field Distribution of Normal Pulsars: Implications for the Multiple Origins for Neutron Stars." Publications of the Astronomical Society of the Pacific 134, no. 1041 (2022): 114201. http://dx.doi.org/10.1088/1538-3873/ac9ad8.

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Abstract In this study, we revisit the magnetic field (B-field) distribution of normal pulsars, motivated by the fact that the number of known pulsars has exceeded 3300. Here, we divided the normal pulsar samples into three subgroups by constant lines of characteristic age τ ch, i.e., young, middle-aged, and old pulsars. We note that τ ch is not used as the time indicator in this study; instead, it just served as cutting lines to divide the pulsar samples. Then, we applied several statistical tests, i.e., the Anderson–Darling, Shapiro–Wilk, Kolmogorov–Smirnov, and Mann–Whitney–Wilcoxon tests,

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Han, JinLin. "Pulsars as excellent probes for the magnetic structure in our Milky Way." Proceedings of the International Astronomical Union 8, S291 (2012): 223–28. http://dx.doi.org/10.1017/s174392131202371x.

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AbstractIn this invited talk, I first discuss the advantages and disadvantages of many probes for the magnetic fields of the Milky Way. I conclude that pulsars are the best probes for the magnetic structure in our Galaxy, because magnetic field strength and directions can be derived from their dispersion measures (DMs) and rotation measures (RMs). Using the pulsars as probes, magnetic field structures in the Galactic disk, especially the field reversals between the arms and interarm regions, can be well revealed from the distribution of RM data. The field strengths on large scales and small sc

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Noutsos, Aristeidis. "Measuring ISM fields using Pulsars." Proceedings of the International Astronomical Union 4, S259 (2008): 15–24. http://dx.doi.org/10.1017/s1743921309030026.

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AbstractThe sample of available Galactic pulsar rotation measures has proven an invaluable tool for measuring the direction and magnitude of the interstellar magnetic fields of our Galaxy. In this review, I present highlights of recent efforts to measure and map the Galactic magnetic field using pulsars. I give an overview of the analysis methods that were used by previous authors and underline the key results that have given us a clear picture of the magnetic field in certain regions of the Galaxy. This review also lays out the limitations of the present analysis methods and the observational

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Cole, K. D. "The Magnetic Fields of Pulsars, Electrons and the Sun." Publications of the Astronomical Society of Australia 10, no. 2 (1992): 110–12. http://dx.doi.org/10.1017/s1323358000019408.

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AbstractAn apparent connection is reported between the magnetic field strengths inside an electron, in newly born pulsars, and the sun. It is argued that the upper limit to the strength of magnetic field which seems to exist is that which would permit emission of a photon at the non-relativistic electron gyrofrequency, with energy of the order of the electron rest mass. The strongest magnetic fields at the surface of polar regions of pulsars conform to this. By equating approximately the rest mass of an electron to its magnetic energy, the same magnetic field is found inside the electron. It i

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Dissertations / Theses on the topic "Magnetic field – pulsars"

1

Zhu, Weiwei. "The cooling of high-magnetic-field pulsars." Thesis, McGill University, 2011. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=104725.

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Prior to ~20 years ago, only two kinds of pulsars were known: RPPs and accretion-powered pulsars. The rapid advance of X-ray astronomy in the past few decades has led to the discovery of magnetic-powered pulsars, namely "magnetars". Magnetars were first identified with the SGRs which exhibit sporadic soft gamma-ray bursts. More recently, another group of pulsars, the AXPs, characterised by their bright persistent X-ray emission that is more powerful than their spin-down luminosity, were also recognized as members of the magnetar family. Both SGRs and AXPs have very high (10¹⁴-10¹⁵ G) magnetic

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Yuen, Rai. "Pulsar Magnetosphere Revisited: Emission Geometry and the Synthesis of the Vacuum-Dipole and the Rotating-Magnetosphere Models." Thesis, The University of Sydney, 2013. http://hdl.handle.net/2123/10011.

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We reconsider the vacuum-dipole model (VDM) and the corotating-magnetosphere model (CMM) for pulsar electrodynamics. Both the VDM and the CMM are fatally flawed as stand-alone models. The former model is used for deriving certain pulsar parameters, such as the surface magnetic field strength and characteristic age, but it lacks the plasma required to emit the observed radiation. The latter model introduces important concepts, such as the Goldreich-Julian charge density and corotation electric field, which form the basis for more detailed models, but it neglects the inductive electric field. Wh

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Kundu, Anu. "Contribution of multipolar electromagnetic fields to the radio and high energy emission of pulsars." Thesis, Strasbourg, 2018. http://www.theses.fr/2018STRAE014/document.

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L'étude du champ électromagnétique autour des étoiles à neutrons est l'une des méthodes vitales pour comprendre la physique des pulsars. Alors que la plupart des publications utilisent l'hypothèse d'un champ électromagnétique dipolaire centré standard, des études récentes se sont concentrées sur l'inclusion de composantes de champ multipolaire plus élevées et ont présenté une image plus générale pour les pulsars dans lesquels le moment du dipôle magnétique est décalé du centre de l'étoile. Ce travail discute des conséquences d'un dipôle magnétique rotatif excentré dans le vide en montrant dive

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Doroshenko, Victor [Verfasser], and Andrea [Akademischer Betreuer] Santangelo. "Magnetic fields of accreting pulsars / Victor Doroshenko ; Betreuer: Andrea Santangelo." Tübingen : Universitätsbibliothek Tübingen, 2011. http://nbn-resolving.de/urn:nbn:de:bsz:21-opus-57289.

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Viganò, Daniele. "Magnetic fields in neutron stars." Doctoral thesis, Universidad de Alicante, 2013. http://hdl.handle.net/10045/36185.

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Gralla, Samuel E., Alexandru Lupsasca, and Alexander Philippov. "PULSAR MAGNETOSPHERES: BEYOND THE FLAT SPACETIME DIPOLE." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/622675.

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Most studies of the pulsar magnetosphere have assumed a pure magnetic dipole in flat spacetime. However, recent work suggests that the effects of general relativity are in fact of vital importance and that realistic pulsar magnetic fields will have a significant nondipolar component. We introduce a general analytical method for studying the axisymmetric force-free magnetosphere of a slowly rotating star of arbitrary magnetic field, mass, radius, and moment of inertia, including all the effects of general relativity. We confirm that spacelike current is generically present in the polar caps (su

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Gralla, Samuel E., Alexandru Lupsasca, and Alexander Philippov. "Inclined Pulsar Magnetospheres in General Relativity: Polar Caps for the Dipole, Quadrudipole, and Beyond." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/626414.

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In the canonical model of a pulsar, rotational energy is transmitted through the surrounding plasma via two electrical circuits, each connecting to the star over a small region known as a "polar cap." For a dipole-magnetized star, the polar caps coincide with the magnetic poles (hence the name), but in general, they can occur at any place and take any shape. In light of their crucial importance to most models of pulsar emission (from radio to X-ray to wind), we develop a general technique for determining polar cap properties. We consider a perfectly conducting star surrounded by a force-free m

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Tartt, Kent A. "Magnetic field-induced absorption of short ultra-intense laser pulses." Thesis, Monterey, Calif. : Springfield, Va. : Naval Postgraduate School ; Available from National Technical Information Service, 2000. http://handle.dtic.mil/100.2/ADA381771.

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Thesis (M.S. in Applied Physics) Naval Postgraduate School, June 2000.<br>Thesis advisor(s): Kruer, William L.; Colson, William B. "June 2000." Includes bibliographical references (p. 39-40). Also available in print.

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Coburn, Wayne. "A study of magnetic fields of accreting x-ray pulsars with the Rossi x-ray timing explorer /." Diss., Connect to a 24 p. preview or request complete full text in PDF format. Access restricted to UC IP addresses, 2001. http://wwwlib.umi.com/cr/ucsd/fullcit?p3015845.

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Dias, André. "Development of a scanning MOKE system with a 10 T pulsed magnetic field source." Thesis, Université Grenoble Alpes (ComUE), 2016. http://www.theses.fr/2016GREAY099.

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Nous avons développé un système de mesure magnéto-optique à balayage basé sur l’Effet Kerr(MOKE). Le montage permet mesurer des cycles d'aimantation en balayant de larges surfaces (150 x 150 mm 2 ) sous un champ magnétique pulsé allant jusqu’à 10 T à température ambiante. Les champs magnétiques intenses sont produits par des bobines millimétriques (diamètre interne = 3 mm) connectées à un générateur de courant bipolaire pulsé. Nous avons pu démontrer que ce système présente un fort potentiel pour l'étude combinatoire de couches magnétiques dures. Pour cela, nous avons dressé grâce à notre syst

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Books on the topic "Magnetic field – pulsars"

1

Tartt, Kent A. Magnetic field-induced absorption of short ultra-intense laser pulses. Naval Postgraduate School, 2000.

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2

M, Cordes James, Yadigaroglu I. -A, and United States. National Aeronautics and Space Administration., eds. X-ray emission from the Guitar Nebula. National Aeronautics and Space Administration, 1997.

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X-ray emission from the Guitar Nebula. National Aeronautics and Space Administration, 1997.

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M, Cordes James, Yadigaroglu I. -A, and United States. National Aeronautics and Space Administration., eds. X-ray emission from the Guitar Nebula. National Aeronautics and Space Administration, 1997.

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X-ray emission from the Guitar Nebula. National Aeronautics and Space Administration, 1997.

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6

Davey, Kent. Magnetic field stimulation: the brain as a conductor. Edited by Charles M. Epstein, Eric M. Wassermann, and Ulf Ziemann. Oxford University Press, 2012. http://dx.doi.org/10.1093/oxfordhb/9780198568926.013.0005.

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For the purposes of magnetic stimulation, the brain can be treated as a homogeneous conductor. A properly designed brain stimulation system starts with the target stimulation depth, and it should incorporate the neural strength–duration response characteristics. Higher-frequency pulses require stronger electric fields. The background of this article is the theoretical base determining, where in the brain TMS induces electrical activity, and whether this shifts as a function of differences in the conductivity and organization of gray matter, white matter, and cerebrospinal fluid. The use of str

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An X-ray pulsar with a superstrong magnetic field in the soft gamma-ray repeater SGR1806-20. National Aeronautics and Space Administration, 1998.

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An X-ray pulsar with a superstrong magnetic field in the soft gamma-ray repeater SGR1806-20. National Aeronautics and Space Administration, 1998.

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Chryssa, Kouveliotou, and United States. National Aeronautics and Space Administration., eds. An X-ray pulsar with a superstrong magnetic field in the soft gamma-ray repeater SGR1806-20. National Aeronautics and Space Administration, 1998.

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Chryssa, Kouveliotou, and United States. National Aeronautics and Space Administration., eds. An X-ray pulsar with a superstrong magnetic field in the soft gamma-ray repeater SGR1806-20. National Aeronautics and Space Administration, 1998.

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Book chapters on the topic "Magnetic field – pulsars"

1

Lyne, A. G. "Pulsars as Probes of the Galactic Magnetic Field." In Galactic and Intergalactic Magnetic Fields. Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0569-6_11.

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Ruderman, M. "Magnetic Field Evolution from Neutron Star Crust Breaking." In X-Ray Binaries and Recycled Pulsars. Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2704-2_42.

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Ikhsanov, N. R., and N. G. Beskrovnaya. "Can the magnetic field of long-period X-ray pulsars be supercritical ?" In High-Energy Emission from Pulsars and their Systems. Springer Berlin Heidelberg, 2010. http://dx.doi.org/10.1007/978-3-642-17251-9_28.

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Pineault, Serge. "The Relation between Radio Luminosity and Magnetic Field in Rotation-Powered Pulsars." In The Origin and Evolution of Neutron Stars. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-3913-4_7.

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Kulkarni, Shrinivas R. "Secondary Components of Binary Pulsars & Magnetic Field Decay in Neutron Stars." In The Origin and Evolution of Neutron Stars. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-3913-4_74.

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Verbunt, Frank. "The Origin and Evolution of X-ray Binaries and Low-Magnetic-Field Radio Pulsars." In Neutron Stars and Their Birth Events. Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0515-3_14.

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Gonzalez, M. E., V. M. Kaspi, F. Camilo, B. M. Gaensler, and M. J. Pivovaroff. "PSR J1119–6127 and the X-ray emission from high magnetic field radio pulsars." In Isolated Neutron Stars: From the Surface to the Interior. Springer Netherlands, 2007. http://dx.doi.org/10.1007/978-1-4020-5998-8_12.

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Noutsos, Aristeidis. "The Magnetic Field of the Milky Way from Faraday Rotation of Pulsars and Extragalactic Sources." In Space Sciences Series of ISSI. Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4614-5728-2_13.

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Beskin, V. S., S. V. Chernov, C. R. Gwinn, and A. A. Tchekhovskoy. "Radio Pulsars." In The Strongest Magnetic Fields in the Universe. Springer New York, 2016. http://dx.doi.org/10.1007/978-1-4939-3550-5_7.

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Asseo, E., G. Pelletier, and H. Sol. "Magnetized Langmuir Solitons Around Pulsars." In Galactic and Intergalactic Magnetic Fields. Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0569-6_7.

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Conference papers on the topic "Magnetic field – pulsars"

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Petit, Véronique, Gregg A. Wade, Laurent Drissen, et al. "Exploring the origin of neutron star magnetic field: magnetic properties of the progenitor OB stars." In 40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More. AIP, 2008. http://dx.doi.org/10.1063/1.2900263.

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Hoyos, Jaime, Andreas Reisenegger, Juan A. Valdivia, et al. "Multi-Fluid Simulation of the Magnetic Field Evolution in Neutron Stars." In 40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More. AIP, 2008. http://dx.doi.org/10.1063/1.2900265.

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Zhang, C. M., C. Bassa, Z. Wang, A. Cumming, and V. M. Kaspi. "On the bottom spin period and magnetic field of millisecond pulsar." In 40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More. AIP, 2008. http://dx.doi.org/10.1063/1.2900297.

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Cumming, A., Rudy Wijnands, Diego Altamirano, et al. "Magnetic Field Evolution in Accreting Millisecond Pulsars." In A DECADE OF ACCRETING MILLISECOND X-RAY PULSARS. AIP, 2008. http://dx.doi.org/10.1063/1.3031186.

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Ng, C. Y., V. M. Kaspi, Ersin Göğüş, Ünal Ertan, and Tomaso Belloni. "High Magnetic Field Rotation-powered Pulsars." In ASTROPHYSICS OF NEUTRON STARS 2010: A Conference in Honor of M. Ali Alpar. AIP, 2011. http://dx.doi.org/10.1063/1.3629486.

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Esposito, P., N. Rea, R. Turolla, et al. "SGR 0418+5729: a low-magnetic-field magnetar." In RADIO PULSARS: AN ASTROPHYSICAL KEY TO UNLOCK THE SECRETS OF THE UNIVERSE. AIP, 2011. http://dx.doi.org/10.1063/1.3615111.

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Payne, D. J. B., M. Vigelius, A. Melatos, et al. "Magnetic field evolution of accreting neutron stars." In A DECADE OF ACCRETING MILLISECOND X-RAY PULSARS. AIP, 2008. http://dx.doi.org/10.1063/1.3031185.

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Safi-Harb, Samar, C. Bassa, Z. Wang, A. Cumming, and V. M. Kaspi. "An X-ray View of the High Magnetic Field Radio Pulsar J1119–6127: Any Link to Magnetars?" In 40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More. AIP, 2008. http://dx.doi.org/10.1063/1.2900145.

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Kaspi, V. M. "Discovery of two high-magnetic-field radio pulsars." In X-RAY ASTRONOMY: Stellar Endpoints,AGN, and the Diffuse X-ray Background. AIP, 2001. http://dx.doi.org/10.1063/1.1434660.

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Gao, Zhi-Fu, Hao Shan, Hui Wang, and Na Wang. "Evolutions of magnetic field and spin-down of pulsars." In XIAMEN-CUSTIPEN WORKSHOP ON THE EQUATION OF STATE OF DENSE NEUTRON-RICH MATTER IN THE ERA OF GRAVITATIONAL WAVE ASTRONOMY. AIP Publishing, 2019. http://dx.doi.org/10.1063/1.5117823.

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Reports on the topic "Magnetic field – pulsars"

1

Afeyan, Bedros. Generation and Control of Self-Organized Nonlinear Kinetic Structures in High Energy Density Plasmas in the Presence of Intense Magnetic Fields and Ultrashort Laser Pulses. Office of Scientific and Technical Information (OSTI), 2022. http://dx.doi.org/10.2172/1895611.

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Shadwick, Bradley. Generation and Control of Self-Organized Nonlinear Kinetic Structures in High Energy Density Plasmas in the Presence of Intense Magnetic Fields and Ultrashort Laser Pulses. Office of Scientific and Technical Information (OSTI), 2022. http://dx.doi.org/10.2172/1894685.

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