Life Unknown: Preliminary Scheme for a Magnetotrophic Organism by Dirk Schulze-Makuch, Louis N. Irwin

“…If the magnetic field strength were much larger, such as that on planets around neutron stars or magnetars, metabolic energy could be obtained from these magnetic fields in principle. …”
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Unitary Limit of Two-Nucleon Interactions in Strong Magnetic Fields by Detmold, William, Orginos, Kostas, Savage, Martin J., Tiburzi, Brian C., Beane, Silas R., Chang, Emmanuel, Parreno, Assumpta

“…Fields of this strength may exist inside magnetars and in peripheral relativistic heavy ion collisions, and the unitary behavior at large scattering lengths may have important consequences for these systems.…”
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The 60 pc Environment of FRB 20180916B by Tendulkar, Shriharsh P, Gil de Paz, Armando, Kirichenko, Aida Yu, Hessels, Jason WT, Bhardwaj, Mohit, Ávila, Fernando, Bassa, Cees, Chawla, Pragya, Fonseca, Emmanuel, Kaspi, Victoria M, Keimpema, Aard, Kirsten, Franz, Lazio, T Joseph W, Marcote, Benito, Masui, Kiyoshi, Nimmo, Kenzie, Paragi, Zsolt, Rahman, Mubdi, Payá, Daniel Reverte, Scholz, Paul, Stairs, Ingrid

“…With the typical projected velocities of pulsars, magnetars, or neutron stars in binaries (60-750 km s−1), FRB 20180916B would need 800 kyr to 7 Myr to traverse the observed distance from its presumed birth site. …”
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Nonperturbative QED vacuum birefringence by V.I. Denisov, E.E. Dolgaya, V.A. Sokolov

“…Such expansion is especially important in astrophysics because magnetic fields of some pulsars and magnetars greatly exceed quantum magnetic field limit, so the estimates of perturbative QED effects in this case require clarification.…”
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General Relativistic Mean-Field Dynamo Model for Proto-Neutron Stars by Kevin Franceschetti, Luca Del Zanna

“…Neutron stars, and magnetars in particular, are known to host the strongest magnetic fields in the Universe. …”
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Olbert’s Kappa Fermi and Bose Distributions by R. A. Treumann, R. A. Treumann, Wolfgang Baumjohann

“…Possible applications are envisaged to condensed matter physics, possibly quantum plasmas, and dense astrophysical objects like the interior state of terrestrial planets, neutron stars, magnetars where quantum effects come into play and dominate the microscopic scale but may have macroscopic consequences.…”
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Future of Neutron Star Studies with Fast Radio Bursts by Sergei B. Popov, Maxim S. Pshirkov

“…Thus, in the following decade we expect to have a very large sample of events directly related to extragalactic magnetars of different origin. This might open new possibilities to probe various aspects of NS physics. …”
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HOT DENSE MAGNETIZED SPINOR MATTER IN PARTICLE AND ASTROPARICLE PHYSICS: THE ROLE OF BOUNDARIES by Yu. A. Sitenko

“…This points at a significant role of boundaries for physical systems with hot dense magnetized spinor matter, i.e. compact astrophysical objects (neutron stars and magnetars), relativistic heavy-ion collisions, novel materials known as the Dirac and Weyl semimetals.…”
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Radio polarization measurements from RRAT J1819-1458 by Karastergiou, A, Hotan, A, Straten, W, McLaughlin, M, Ord, S

“…We compare these polarization properties to those of other radio emitting neutron star populations, including young pulsars, pulsars with a high surface magnetic field and radio emitting magnetars. From the polarization measurements, the Faraday rotation measure of this RRAT is derived.…”

Einstein–Cartan–Dirac gravity with U(1) symmetry breaking by Francisco Cabral, Francisco S. N. Lobo, Diego Rubiera-Garcia

“…In particular, we briefly address some astrophysical considerations regarding the relevance of the effects which might take place inside ultra-dense neutron stars with strong magnetic fields (magnetars).…”
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Laboratory evidence of dynamo amplification of magnetic fields in a turbulent plasma by Tzeferacos, P, Rigby, A, Bott, A, Bell, A, Bingham, R, Casner, A, Cattaneo, F, Churazov, EM, Emig, J, Fiuza, F, Forest, CB, Foster, J, Graziani, C, Katz, J, Koenig, M, Li, CK, Meinecke, J, Petrasso, R, Park, HS, Remington, BA, Ross, JS, Ryu, D, Ryutov, D, White, TG, Reville, B, Miniati, F, Schekochihin, A, Lamb, DQ, Froula, DH, Gregori, G

“…Diffuse radiosynchrotron emission observations and Faraday rotation measurements have revealed magnetic field strengths ranging from a few nG and tens of µG in extragalactic disks, halos and clusters [1], up to hundreds of TG in magnetars, as inferred from their spin-down [2]. The energy density of these fields is typically comparable to the energy density of the fluid motions of the plasma in which they are embedded, making magnetic fields essential players in the dynamics of the luminous matter. …”

Critical end point and universality class of neutron ^{3}P_{2} superfluids in neutron stars by Takeshi Mizushima, Shigehiro Yasui, Muneto Nitta

“…This implies that the GL theory can provide a tractable way for understanding critical phenomena which may be realized in the dense core of realistic magnetars.…”
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Radio polarization measurements from RRAT J1819-1458 by Karastergiou, A, Hotan, A, van Straten, W, McLaughlin, M, Ord, S

“…We compare these polarization properties to those of other radio-emitting neutron star populations, including young pulsars, pulsars with a high surface magnetic field and radio-emitting magnetars. From the polarization measurements, the Faraday rotation measure of this rotating radio transient is derived. © 2009 The Authors. …”

Discovery of a radio-emitting neutron star with an ultra-long spin period of 76 s by Caleb, M, Heywood, I, Rajwade, K, Malenta, M, Stappers, B, Barr, E, Chen, W, Morello, V, Sanidas, S, van den Eijnden, J, Kramer, M, Buckley, D, Brink, J, Motta, SE, Woudt, P, Weltevrede, P, Jankowski, F, Surnis, M, Buchner, S, Bezuidenhout, MC, Driessen, LN, Fender, R

“…Our discovery establishes the existence of ultra-long period neutron stars, suggesting a possible connection to the evolution of highly magnetized neutron stars, ultra-long period magnetars, and fast radio bursts.…”

A strategy to unveil transient sources of ultra-high-energy cosmic rays by Takami Hajime

“…Transient generation of ultra-high-energy cosmic rays (UHECRs) has been motivated from promising candidates of UHECR sources such as gamma-ray bursts, flares of active galactic nuclei, and newly born neutron stars and magnetars. Here we propose a strategy to unveil transient sources of UHECRs from UHECR experiments. …”
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Axion-polaritons in quark stars: a possible solution to the missing pulsar problem by E. J. Ferrer, V. de la Incera

“…In the proposed mechanism, the absence of young magnetars occurs because as electromagnetic waves inside the star can only propagate through the hybridized modes, incident photons coming from a $$\gamma $$ γ -ray burst get transformed into massless and massive axion polaritons by the Primakoff effect. …”
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A Search for Magnetized Quark Nuggets (MQNs), a Candidate for Dark Matter, Accumulating in Iron Ore by J. Pace VanDevender, T. Sloan, Michael Glissman

“…Indirect evidence of MQNs has been previously inferred from observations of magnetars and of non-meteorite impact craters. It is shown in this paper that MQNs can accumulate in taconite (iron ore) and be transferred into ferromagnetic rod-mill liners during processing of the ore. …”
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A Short Survey of Matter-Antimatter Evolution in the Primordial Universe by Johann Rafelski, Jeremiah Birrell, Andrew Steinmetz, Cheng Tao Yang

“…We suggest but do not explore further that the methods used in exploring the early Universe may also provide new insights in the study of exotic stellar cores, magnetars, as well as gamma-ray burst (GRB) events. …”
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Stellar mergers as the origin of magnetic massive stars by Schneider, FRN, Ohlmann, ST, Podsiadlowski, P, Röpke, FK, Balbus, SA, Pakmor, R, Springel, V

“…Such massive blue straggler stars seem likely to be progenitors of magnetars, perhaps giving rise to some of the enigmatic fast radio bursts observed11, and their supernovae may be affected by their strong magnetic fields12.…”

IMPLICATIONS FOR THE ORIGIN OF GRB 051103 FROM LIGO OBSERVATIONS by Barnum, Sam, Barsotti, Lisa, Blackburn, Lindy L., Bodiya, Timothy Paul, Corbitt, Thomas R., Donovan, Frederick J., Dwyer, S., Evans, Matthew J., Foley, S., Fritschel, Peter K., Harry, Gregory, Hughey, B., Katsavounidis, Erotokritos, MacInnis, Myron E., Mason, Kenneth R., Matichard, Fabrice, Mavalvala, Nergis, Mittleman, Richard K., Shapiro, B., Shoemaker, David H., Smith, N. D., Soto, J., Stein, A. J., Waldman, S. J., Weiss, Rainer, Wipf, Christopher, Zucker, Michael E.

“…If the event occurred in M81, then our findings support the hypothesis that GRB 051103 was due to an SGR giant flare, making it one of the most distant extragalactic magnetars observed to date.…”
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