REVIEW 3 major objections 5 minor 99 references
Particle Injection Problem in Magnetic Reconnection and Turbulence
T0 review · 3 major / 5 minor · reviewed 2026-08-15 · deepseek-v4-flash
Pith's one-line read Particle injection in magnetic reconnection and turbulence is achieved by Fermi reflection, direct acceleration, and pickup—not by the E>B diffusion regions.
desk verdict A useful, opinionated review whose qualitative point about E>B regions is strong, but whose quantitative injection shares are convention-dependent and should not be taken as the final word. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The machinery that carries the argument is the injection-share classification of Eq. (5). At the first time step a tracer particle attains energy $\gamma > \gamma_{\rm inj}$, the particle is assigned to one of three mechanisms by comparing the parallel and perpendicular energy gains ($W_\parallel$ vs $W_\perp$) and the particle momenta in the simulation frame versus the $E\times B$ drift frame: $E_{\rm rec}$ acceleration if $W_\parallel > W_\perp$ and $|p_\parallel| > |p'_\perp|$; Fermi kick if $W_\perp > W_\parallel$ and $|p_\parallel| > |p'_\perp|$; pickup if $W_\perp > W_\parallel$ and $|p'_\perp| > |p_\parallel|$. These are supplied by the analytic energy-gain estimates of Eqs. (2)–(4): $W_{\rm direct}/m_e c^2 \simeq 0.1\,\omega_{ce}\tau$ for direct acceleration, $W_{\rm Fermi}/m_e c^2 = 2\sigma/(1+\sigma b_g^2)$ for a Fermi reflection, and $W_{\rm pickup}/m_e c^2 = \gamma_{Ax} - \gamma_0$ for pickup. The classification converts 'what injects particles' into countable population shares, and the efficiencies $\eta_N$ and $\eta_E$ of Eq. (6) convert the injection threshold into the thermal–nonthermal energy partition.
What would settle it
In a weakly guided relativistic reconnection simulation, compute injection shares using Eq. (5) and also using a time-resolved decomposition in which each particle's work is split between mechanisms proportionally to the energy gained from each in every time step before $\gamma_{\rm inj}$ is reached; if the time-resolved shares differ materially from the single-label shares (for instance, if most particles receive comparable energy from $E_\parallel$ and $E_\perp$ during injection), then the claim that a dominant primary mechanism exists would be falsified.
Extended reading notes
Core claim
The paper's central claim is that the primary injection of particles in relativistic magnetic reconnection is accomplished by three mechanisms operating outside the E>B diffusion regions—direct acceleration by the reconnection electric field near X-points, a single Fermi reflection off the relaxing field lines in the exhaust (energy gain $W_{\rm Fermi}/m_e c^2 = 2\sigma/(1+\sigma b_g^2)$), and pickup acceleration in the outflow (energy gain $W_{\rm pickup}/m_e c^2 = \gamma_{Ax} - \gamma_0$). Tracing particles in PIC simulations, the paper labels each particle at its first crossing of the injection energy $\gamma_{\rm inj}$ and reports that for weak guide fields Fermi reflection and pickup dominate, direct acceleration is competitive at high magnetization, and parallel electric fields dominate only when the guide field is strong ($b_g \gtrsim 1$). The number and energy injection efficiencies in the weak-guide-field, high-magnetization case are approximately 40% and 90%, respectively, implying an efficient thermal-to-nonthermal conversion. The same multi-mechanism picture is extended to nonrelativistic and transrelativistic reconnection and to magnetically dominated turbulence, where parallel and perpendicular electric fields contribute comparably and the perpendicular contribution grows with system size.
Load-bearing premise
The claim that we know which mechanism injects each particle rests on the assumption that a single mechanism can be unambiguously identified from the particle's parallel versus perpendicular energy gain and momenta at the moment it crosses the injection threshold, even though particles can be accelerated by parallel and perpendicular fields simultaneously.
Editorial extensions
If this is right
- Large-scale particle acceleration models that couple MHD reconnection with test particles can treat injection as a small set of localized channels (Fermi reflection at exhausts, direct acceleration near X-points, pickup in outflows) and can ignore resolving kinetic E>B diffusion regions.
- Injection efficiency directly determines the observable thermal–nonthermal partition: up to about 40% of particles and 90% of energy in weak-guide-field relativistic reconnection, decreasing to about 15% and 60%, respectively, as the guide field reaches $b_g = 1$.
- Judging an injection mechanism by the highest-energy particles overestimates the role of parallel electric fields; the primary mechanism should be the one that explains the majority of injected particles above $\varepsilon_{\rm inj}$.
- In relativistic turbulence, the injection shares of parallel and perpendicular electric fields are comparable, and the perpendicular contribution increases with system size, so small kinetic simulations understate the role of motional electric fields.
- In proton–electron plasmas, ions are injected mainly by perpendicular (motional) electric fields while electrons depend more on parallel (non-ideal) fields, which sets the relative abundance of species in the nonthermal population.
Reading between the lines
- The review implies a testable dichotomy: if exhaust-crossing Fermi reflections are the dominant injection channel, then particle energy gains in spacecraft observations (e.g., in Earth's magnetotail) should correlate with exhaust crossings rather than with time spent in E>B regions; this correlation has not yet been measured.
- The exclusive-label classification of Eq. (5) could be probed by a soft classification that splits each particle's work proportionally between mechanisms up to the injection time; large discrepancies between the two share estimates would indicate that the notion of a single dominant mechanism is not robust.
- The reported efficiencies depend on the fitted value of $\gamma_{\rm inj}$; propagating the fit uncertainty into $\eta_N$ and $\eta_E$ would convert the 40%/90% numbers into ranges that can be compared across simulation codes and guide-field values.
- A population-level extension would embed the three analytic energy gains (Eqs. 2–4) into a model where injection is sampled from these channels and followed by Fermi acceleration; the predicted power-law index and thermal fraction could then be compared with full PIC spectra as a consistency check.
Signed reviews
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. This review paper addresses the particle injection problem in magnetic reconnection and turbulence: how thermal particles are pre-accelerated to the lower bound of a nonthermal power-law spectrum. The authors argue that the diffusion regions where |E|>|B| are not the primary injection channel, based on dwell-time statistics, direct energy-gain measurements, and a test-particle experiment that removes electric fields in E>B regions. They instead attribute injection to three mechanisms—direct acceleration by the non-ideal electric field, Fermi reflection, and pickup acceleration—and quantify their relative contributions using a classification rule in Eq. (5). They report injection efficiencies reaching roughly 40% in particle number and 90% in energy for weak-guide-field relativistic reconnection, and they survey companion regimes: nonrelativistic and transrelativistic reconnection, and relativistic turbulence. The review closes with an outlook emphasizing that kinetic diffusion regions may be ignored in macroscopic particle acceleration models and that injection models are needed for global-scale simulations.
Significance. If the synthesis holds, it would settle an active controversy (Sironi and Spitkovsky vs. Guo et al.) about whether E>B regions are essential for injection, and it would provide concrete input for large-scale and macroscopic particle acceleration models that cannot resolve kinetic scales. The paper's strengths include: a clear presentation of the competing claims; a falsifiable test-particle experiment (Fig. 2c) supporting the claim that E>B electric fields are not necessary for injection; closed-form energy-gain estimates for three mechanisms (Eqs. 2-4); and a cross-regime review that connects relativistic reconnection, nonrelativistic reconnection, and turbulence. The main weakness is that the quantitative injection shares, which are central to the 'primary mechanism' conclusion, rest on a winner-take-all classification rule that the paper itself shows to be convention-dependent. The E>B claim is more robust than the share decomposition, and the paper's practical conclusion about ignoring kinetic diffusion regions is defensible.
major comments (3)
- [§2.2, Eq. (5) and Figs. 4-5, 11] The classification of injection mechanisms is winner-take-all and convention-dependent. Eq. (5) assigns each particle to exactly one mechanism at the first crossing of gamma_inj using inequalities between W_parallel and W_perp and between |p_parallel| and |p'_perp|. The paper itself shows the resulting shares are not unique: Fig. 5 compares this decomposition with W_n vs W_m and W_E>B vs W_E<B and obtains different quantitative shares, and Fig. 11(c,d) shows parallel and perpendicular work acting simultaneously during injection, with the caption stating that 'for many particles classification of the injection mechanism is not straight forward.' Because the reported ordering of mechanisms in Fig. 4 and the associated efficiency statements depend on this arbitrary labeling, the central quantitative synthesis is conditional on the chosen rule. The review should either explicitly frame the shares as one specific decomposition, provide a sensitivity analysis (e.g., fractional attribution or variation of the threshold), or soften the 'primary mechanism' claims accordingly.
- [§2.1, Eq. (1)] The dwell-time argument for why E>B regions cannot inject most particles uses the inequality Delta_gamma_E>B <= integral of q r B0 c dt/(m_e c^2) with r ~ 0.1. As written, this bounds only acceleration by a reconnection electric field of magnitude r B0, but in E>B regions the electric field can locally exceed this value by definition (E/B > 1), so Eq. (1) is not a rigorous upper bound on all energy gain inside E>B regions. The conclusion is nevertheless supported by the direct energy-gain distribution in Fig. 2b and by the test-particle experiment in Fig. 2c. The text should present Eq. (1) as an estimate for one specific acceleration channel and rely on the measured energy gains for the global claim.
- [§2.3 and §5] The quantitative efficiency numbers—up to 40% number efficiency and 90% energy efficiency in weak-guide-field relativistic reconnection—depend on the fitted injection energy epsilon_inj. The paper notes in Section 5 that 'conclusions can be very different if lower energy particles are included as the nonthermals,' but this caveat is not reflected in the efficiency definitions or in how the numbers are presented in Fig. 6. Given that these numbers are likely to be extracted and used in applications, the review should quantify the sensitivity of eta_N and eta_E to the spectral fitting procedure and to the choice of epsilon_inj, or at least explicitly state the expected uncertainty in the reported efficiencies.
minor comments (5)
- [§2.1, Fig. 2c] The test-particle experiment in Fig. 2c is one of the strongest pieces of evidence in the review; the text mentions 84% (94%) for gamma_inj = sigma (sigma/4) but does not state the error bar or the number of particles used. Reporting the statistical uncertainty would strengthen the claim.
- [§2.2, Eq. (3)] The Fermi energy-gain formula is correct, but the notation b_g is introduced earlier without an explicit definition at first use in the text; it is defined in the Introduction, but a brief reminder in Section 2.2 would help readability.
- [§4, Fig. 18] The caption says the figure shows the 'share of the work done by the parallel electric field' before and after injection, but the axes labels are not clearly described in the text. Please specify the normalization and the exact definition of 'share' used in that figure.
- [§5] The sentence 'The role of non-ideal electric field when a guide field is present and when it is proton-electron plasmas' is grammatically incomplete and should be finished.
- [References] Some key references are cited as 'in preparation' or arXiv-only (e.g., French et al. [81], Singh et al. [80]). For a review, provide published versions or note their status explicitly so readers can assess reproducibility.
Circularity Check
No significant circularity: the review is a data-driven synthesis that explicitly discloses the convention-dependence of its injection classification.
full rationale
This paper is a review, not a derivation, and its central quantitative claims are either direct measurements from PIC simulations or kinematic estimates with clearly stated assumptions. The injection-share decomposition in Eq. (5) is explicitly presented as a categorization scheme: particles are 'categorized to a mechanism based on the following criteria,' so the reported shares are transparently defined by that rule rather than derived from a hidden input. The paper further acknowledges in Fig. 5 and Section 5 that different decomposition choices (W_n vs. W_m, W_E>B vs. W_E<B, and even the inclusion of lower-energy particles) can change the conclusions, so the classification is disclosed as convention-dependent rather than smuggled in as a prediction. The E>B insufficiency argument in Sec. 2.1 uses an independent physical estimate (Eq. 1) compared against simulation-measured residence times, and it is robust to two different choices of gamma_inj. The injection energy gamma_inj is fitted from spectra, but it is used as a measured threshold to quantify efficiencies, not renamed as a prediction. Self-citations refer to published simulations by the same group, but the review also engages external works (Sironi, Totorica, Gupta) and does not rely on any uniqueness theorem or ansatz imported solely from the authors' prior work. No step in the paper's argument reduces by construction to its own inputs, so no significant circularity is present.
Assumptions & free parameters
free parameters (2)
- injection energy threshold epsilon_inj =
varies with regime (e.g., sigma/4, sigma, 10, sigma/2, 0.2-0.5 m_p v_A^2)
- reconnection rate R =
0.1
assumptions (3)
- domain assumption PIC simulations provide a first-principles description of plasma dynamics and particle acceleration.
- ad hoc to paper The classification criteria in Eq. (5) map each particle to a single injection mechanism.
- standard math The Fermi reflection energy gain formula in Eq. (3) applies to the reconnection exhaust geometry.
Cite this review
Pith. "Pith review of Particle Injection Problem in Magnetic Reconnection and Turbulence." pith.science (2026). https://pith.science/paper/Z3WT4VZM
@misc{pith2026250619938,
author = {Pith},
title = {Pith review of: Particle Injection Problem in Magnetic Reconnection and Turbulence},
year = {2026},
howpublished = {\url{https://pith.science/paper/Z3WT4VZM}},
note = {Machine review of arXiv:2506.19938}
}
read the original abstract
Magnetic reconnection and turbulence in magnetically-dominated environments have been proposed as important nonthermal particle acceleration mechanisms that generate high energy particles and associated emissions. While the acceleration to high energy that produces the power-law energy distribution has drawn strong interest, recent studies actively discuss pre-acceleration, or injection, to a sufficient energy for a sustained and prolonged Fermi-like acceleration. The injection process is important for determining the fraction of nonthermal particles and energy partition between thermal and nonthermal particles. We review recent advances in understanding the injection mechanisms responsible for populating these nonthermal power-law spectra, and conclude with an outlook for studies and applications of injection models.
Reference graph
Works this paper leans on
-
[1]
Physics Report154(1), 1–75 (1987) https://doi.org/10
Blandford, R., Eichler, D.: Particle acceleration at astrophysical shocks: A theory of cosmic ray origin. Physics Report154(1), 1–75 (1987) https://doi.org/10. 1016/0370-1573(87)90134-7
1987
-
[2]
Abeysekara, A.U., Albert, A., Alfaro, R., Alvarez, C., ´Alvarez, J.D., Arceo, R., Arteaga-Vel´ azquez, J.C., Avila Rojas, D., Ayala Solares, H.A., Barber, A.S., Bautista-Elivar, N., Becerril, A., Belmont-Moreno, E., BenZvi, S.Y., Berley, D., Bernal, A., Braun, J., Brisbois, C., Caballero-Mora, K.S., Capistr´ an, T., Carrami˜ nana, A., Casanova, S., Castil...
arXiv 2017
-
[3]
Chen, B., Shen, C., Gary, D.E., Reeves, K.K., Fleishman, G.D., Yu, S., Guo, F., Krucker, S., Lin, J., Nita, G.M., Kong, X.: Measurement of magnetic field and relativistic electrons along a solar flare current sheet. Nature Astronomy4, 1140–1147 (2020) https://doi.org/10.1038/s41550-020-1147-7 arXiv:2005.12757 [astro-ph.SR]
arXiv 2020
-
[4]
Space Science Reviews90, 413–491 (1999) https://doi.org/10.1023/A:1005105831781 21
Reames, D.V.: Particle acceleration at the Sun and in the heliosphere. Space Science Reviews90, 413–491 (1999) https://doi.org/10.1023/A:1005105831781 21
-
[5]
Li, X., Guo, F., Liu, Y.-H.: The acceleration of charged particles and for- mation of power-law energy spectra in nonrelativistic magnetic reconnection. Physics of Plasmas28(5), 052905 (2021) https://doi.org/10.1063/5.0047644 arXiv:2104.10732 [physics.plasm-ph]
arXiv 2021
-
[6]
Oka, M., Birn, J., Egedal, J., Guo, F., Ergun, R.E., Turner, D.L., Khotyaintsev, Y., Hwang, K.-J., Cohen, I.J., Drake, J.F.: Particle Acceleration by Magnetic Reconnection in Geospace. Space Science Reviews219(8), 75 (2023) https:// doi.org/10.1007/s11214-023-01011-8 arXiv:2307.01376 [physics.space-ph]
arXiv 2023
-
[7]
Guo, F., Liu, Y.-H., Zenitani, S., Hoshino, M.: Magnetic Reconnection and Associated Particle Acceleration in High-Energy Astrophysics. Space Sci- ence Reviews220(4), 43 (2024) https://doi.org/10.1007/s11214-024-01073-2 arXiv:2309.13382 [astro-ph.HE]
arXiv 2024
-
[8]
Maximum Energy of Particles in Plasmas
Oka, M., Makishima, K., Terasawa, T.: Maximum Energy of Particles in Plasmas. Astrophysical Journal979(2), 161 (2025) https://doi.org/10.3847/ 1538-4357/ad9916 arXiv:2412.00564 [astro-ph.HE]
work page Pith review arXiv 2025
Show all 99 references
-
[9]
Space Science Reviews221(2), 27 (2025) https://doi.org/10.1007/ s11214-025-01153-x
Drake, J.F., Antiochos, S.K., Bale, S.D., Chen, B., Cohen, C.M.S., Dahlin, J.T., Glesener, L., Guo, F., Hoshino, M., Imada, S., Oka, M., Phan, T.D., Reeves, K.K., Swisdak, M.: Magnetic Reconnection in Solar Flares and the Near-Sun Solar Wind. Space Science Reviews221(2), 27 (2...
2025
-
[10]
Fermi, E.: On the origin of the cosmic radiation. Phys. Rev.75, 1169–1174 (1949) https://doi.org/10.1103/PhysRev.75.1169
1949 doi
-
[11]
Monthly Notices of the Royal Astronomical Society182, 147–156 (1978) https://doi.org/10.1093/ mnras/182.2.147
Bell, A.R.: The acceleration of cosmic rays in shock fronts - I. Monthly Notices of the Royal Astronomical Society182, 147–156 (1978) https://doi.org/10.1093/ mnras/182.2.147
1978
-
[12]
Astronomy and Astrophysics347, 370–374 (1999) https://doi.org/10.48550/arXiv.astro-ph/9905178 arXiv:astro- ph/9905178 [astro-ph]
Drury, L.O., Duffy, P., Eichler, D., Mastichiadis, A.: On “box” models of shock acceleration and electron synchrotron spectra. Astronomy and Astrophysics347, 370–374 (1999) https://doi.org/10.48550/arXiv.astro-ph/9905178 arXiv:astro- ph/9905178 [astro-ph]
-
[14]
Physical Review Letters121(25), 255101 (2018) https://doi.org/10.1103/ PhysRevLett.121.255101 arXiv:1809.01168 [astro-ph.HE]
Comisso, L., Sironi, L.: Particle Acceleration in Relativistic Plasma Turbu- lence. Physical Review Letters121(25), 255101 (2018) https://doi.org/10.1103/ PhysRevLett.121.255101 arXiv:1809.01168 [astro-ph.HE]
2018 arXiv
-
[15]
Physical Review D99(8) (2019) 22 https://doi.org/10.1103/physrevd.99.083006
Lemoine, M.: Generalized fermi acceleration. Physical Review D99(8) (2019) 22 https://doi.org/10.1103/physrevd.99.083006
2019 doi
-
[16]
Monthly Notices of the Royal Astronomical Society499(4), 4972–4983 (2020) https://doi.org/10.1093/mnras/staa3131
Lemoine, M., Malkov, M.A.: Power-law spectra from stochastic acceleration. Monthly Notices of the Royal Astronomical Society499(4), 4972–4983 (2020) https://doi.org/10.1093/mnras/staa3131
2020 doi
-
[17]
Astro- physical Journal948(1), 19 (2023) https://doi.org/10.3847/1538-4357/acb7dd arXiv:2210.08358 [astro-ph.HE]
French, O., Guo, F., Zhang, Q., Uzdensky, D.A.: Particle Injection and Non- thermal Particle Acceleration in Relativistic Magnetic Reconnection. Astro- physical Journal948(1), 19 (2023) https://doi.org/10.3847/1538-4357/acb7dd arXiv:2210.08358 [astro-ph.HE]
2023 arXiv
-
[18]
Astrophysi- cal Journal773(2), 158 (2013) https://doi.org/10.1088/0004-637X/773/2/158 arXiv:1303.5174 [astro-ph.HE]
Guo, F., Giacalone, J.: The Acceleration of Thermal Protons at Paral- lel Collisionless Shocks: Three-dimensional Hybrid Simulations. Astrophysi- cal Journal773(2), 158 (2013) https://doi.org/10.1088/0004-637X/773/2/158 arXiv:1303.5174 [astro-ph.HE]
2013 arXiv
-
[19]
Astrophysical Journal974(1), 47 (2024) https://doi.org/10.3847/1538-4357/ ad6561 arXiv:2404.08807 [astro-ph.SR]
Zhang, Q., Guo, F., Daughton, W., Li, X., Li, H.: Plasma Dynamics and Non- thermal Particle Acceleration in 3D Nonrelativistic Magnetic Reconnection. Astrophysical Journal974(1), 47 (2024) https://doi.org/10.3847/1538-4357/ ad6561 arXiv:2404.08807 [astro-ph.SR]
2024 arXiv
-
[20]
Astro- physical Journal886(2), 122 (2019) https://doi.org/10.3847/1538-4357/ab4c33 arXiv:1909.01420 [astro-ph.HE]
Comisso, L., Sironi, L.: The Interplay of Magnetically Dominated Turbu- lence and Magnetic Reconnection in Producing Nonthermal Particles. Astro- physical Journal886(2), 122 (2019) https://doi.org/10.3847/1538-4357/ab4c33 arXiv:1909.01420 [astro-ph.HE]
2019 arXiv
-
[21]
Astrophysical Journal Letters798(2), 28 (2015) https://doi.org/10.1088/2041-8205/798/2/L28 arXiv:1409.8291 [astro- ph.HE]
Caprioli, D., Pop, A.-R., Spitkovsky, A.: Simulations and Theory of Ion Injection at Non-relativistic Collisionless Shocks. Astrophysical Journal Letters798(2), 28 (2015) https://doi.org/10.1088/2041-8205/798/2/L28 arXiv:1409.8291 [astro- ph.HE]
2015 arXiv
-
[23]
The Astrophysical Journal946(2), 77 (2023) https://doi.org/10
Hoshino, M.: Energy partition of thermal and nonthermal particles in magnetic reconnection. The Astrophysical Journal946(2), 77 (2023) https://doi.org/10. 3847/1538-4357/acbfb5
2023
-
[24]
The Astrophysical Journal818(L9), 7 (2016) https://doi.org/10.3847/ 2041-8205/818/1/L9 23
Guo, F., Li, X., Li, H., Daughton, W., Zhang, B., Lloyd-Ronning, N., Liu, Y.-H., Zhang, H., Deng, W.: Efficient production of high-energy nonthermal par- ticles during magnetic reconnection in a magnetically dominated ion–electron plasma. The Astrophysical Journal818(L9), 7 (2...
2016
-
[26]
Astrophysical Journal Letters936(2), 27 (2022) https://doi.org/10
Comisso, L., Sironi, L.: Ion and Electron Acceleration in Fully Kinetic Plasma Turbulence. Astrophysical Journal Letters936(2), 27 (2022) https://doi.org/10. 3847/2041-8213/ac8422 arXiv:2209.04475 [astro-ph.HE]
2022 arXiv
-
[27]
Physical Review Letters132(11), 115201 (2024) https://doi.org/ 10.1103/PhysRevLett.132.115201 arXiv:2210.04113 [astro-ph.SR]
Zhang, Q., Guo, F., Daughton, W., Li, H., Le, A., Phan, T., Desai, M.: Mul- tispecies Ion Acceleration in 3D Magnetic Reconnection with Hybrid-Kinetic Simulations. Physical Review Letters132(11), 115201 (2024) https://doi.org/ 10.1103/PhysRevLett.132.115201 arXiv:2210.04113 [a...
2024 arXiv
-
[28]
Astrophysical Journal352, 376 (1990) https://doi.org/10.1086/168544
Ellison, D.C., Moebius, E., Paschmann, G.: Particle Injection and Accelera- tion at Earth’s Bow Shock: Comparison of Upstream and Downstream Events. Astrophysical Journal352, 376 (1990) https://doi.org/10.1086/168544
1990 doi
-
[29]
Geophysical Research Letters19(5), 433–436 (1992) https://doi.org/10.1029/92GL00379
Giacalone, J., Burgess, D., Schwartz, S.J., Ellison, D.C.: Hybrid simulations of protons strongly accelerated by a parallel collisionless shock. Geophysical Research Letters19(5), 433–436 (1992) https://doi.org/10.1029/92GL00379
1992 doi
-
[30]
Journal of Physics G Nuclear Physics27(7), 1589–1595 (2001) https://doi.org/ 10.1088/0954-3899/27/7/316 arXiv:astro-ph/0101175 [astro-ph]
Kirk, J.G., Dendy, R.O.: Shock acceleration of cosmic rays - a critical review. Journal of Physics G Nuclear Physics27(7), 1589–1595 (2001) https://doi.org/ 10.1088/0954-3899/27/7/316 arXiv:astro-ph/0101175 [astro-ph]
2001 arXiv
-
[31]
Parsons, J., Spitkovsky, A., Vanthieghem, A.: Microphysics of Particle Reflection in Weibel-Mediated Shocks (2023)
2023
-
[32]
The Astrophysical Journal562(1), 63–66 (2001) https://doi.org/10.1086/337972
Zenitani, S., Hoshino, M.: The generation of nonthermal particles in the relativis- tic magnetic reconnection of pair plasmas. The Astrophysical Journal562(1), 63–66 (2001) https://doi.org/10.1086/337972
2001 doi
-
[33]
Physical Review Letters95(9), 095001 (2005) https://doi.org/10.1103/PhysRevLett.95.095001 arXiv:astro-ph/0505493 [astro-ph]
Zenitani, S., Hoshino, M.: Three-Dimensional Evolution of a Relativistic Current Sheet: Triggering of Magnetic Reconnection by the Guide Field. Physical Review Letters95(9), 095001 (2005) https://doi.org/10.1103/PhysRevLett.95.095001 arXiv:astro-ph/0505493 [astro-ph]
2005 arXiv
-
[34]
Astrophysi- cal Journal770(2), 147 (2013) https://doi.org/10.1088/0004-637X/770/2/147 arXiv:1302.6247 [astro-ph.HE]
Cerutti, B., Werner, G.R., Uzdensky, D.A., Begelman, M.C.: Simulations of Particle Acceleration beyond the Classical Synchrotron Burnoff Limit in Magnetic Reconnection: An Explanation of the Crab Flares. Astrophysi- cal Journal770(2), 147 (2013) https://doi.org/10.1088/0004-63...
2013 arXiv
-
[35]
The Astrophysical Journal783(1), 21 (2014) https://doi.org/ 24 10.1088/2041-8205/783/1/l21
Sironi, L., Spitkovsky, A.: Relativistic reconnection: An efficient source of non- thermal particles. The Astrophysical Journal783(1), 21 (2014) https://doi.org/ 24 10.1088/2041-8205/783/1/l21
2014 doi
-
[36]
Astronomy & Astrophysics570, 111 (2014) https: //doi.org/10.1051/0004-6361/201424083
Melzani, M., Walder, R., Folini, D., Winisdoerffer, C., Favre, J.M.: Relativis- tic magnetic reconnection in collisionless ion-electron plasmas explored with particle-in-cell simulations. Astronomy & Astrophysics570, 111 (2014) https: //doi.org/10.1051/0004-6361/201424083
2014 doi
-
[37]
ApJ806, 167 (2015) https://doi.org/ 10.1088/0004-637X/806/2/167
Guo, F., Liu, Y.-H., Daughton, W., Li, H. ApJ806, 167 (2015) https://doi.org/ 10.1088/0004-637X/806/2/167
2015 doi
-
[38]
ApJ879(L23), 5 (2019) https://doi.org/10.3847/2041-8213/ab2a15
Guo, F., Li, X., Daughton, W., Kilian, P., Li, H., Liu, Y.-H., Yan, W., Ma, D. ApJ879(L23), 5 (2019) https://doi.org/10.3847/2041-8213/ab2a15
2019 doi
-
[39]
The Astrophysical Journal Letters816(1), 8 (2016) https://doi.org/10.3847/2041-8205/816/1/L8
Werner, G.R., Uzdensky, D.A., Cerutti, B., Nalewajko, K., Begelman, M.C.: The extent of power-law energy spectra in collisionless relativistic magnetic recon- nection in pair plasmas. The Astrophysical Journal Letters816(1), 8 (2016) https://doi.org/10.3847/2041-8205/816/1/L8
2016 doi
-
[40]
The Astrophysical Journal Letters 843(2), 27 (2017) https://doi.org/10.3847/2041-8213/aa7892
Werner, G.R., Uzdensky, D.A.: Nonthermal particle acceleration in 3d relativis- tic magnetic reconnection in pair plasma. The Astrophysical Journal Letters 843(2), 27 (2017) https://doi.org/10.3847/2041-8213/aa7892
2017 doi
-
[41]
Monthly Notices of the Royal Astronomical Society473(4), 4840–4861 (2018) https://doi.org/10.1093/mnras/stx2530
Werner, G.R., Uzdensky, D.A., Begelman, M.C., Cerutti, B., Nalewajko, K.: Non-thermal particle acceleration in collisionless relativistic electron–proton reconnection. Monthly Notices of the Royal Astronomical Society473(4), 4840–4861 (2018) https://doi.org/10.1093/mnras/stx2530
2018 doi
-
[42]
The Astrophysical Journal870(1), 49 (2019) https://doi.org/10.3847/ 1538-4357/aaf1b9
Schoeffler, K.M., Grismayer, T., Uzdensky, D., Fonseca, R.A., Silva, L.O.: Bright gamma-ray flares powered by magnetic reconnection in QED-strength magnetic fields. The Astrophysical Journal870(1), 49 (2019) https://doi.org/10.3847/ 1538-4357/aaf1b9
2019
-
[43]
Monthly Notices of the Royal Astronomical Society 498(1), 799–820 (2020) https://doi.org/10.1093/mnras/staa2346
Mehlhaff, J.M., Werner, G.R., Uzdensky, D.A., Begelman, M.C.: Kinetic beam- ing in radiative relativistic magnetic reconnection: a mechanism for rapid gamma-ray flares in jets. Monthly Notices of the Royal Astronomical Society 498(1), 799–820 (2020) https://doi.org/10.1093/mnr...
2020 doi
-
[44]
The Astrophysical Journal912(1), 48 (2021) https://doi.org/10.3847/1538-4357/abedac
Hakobyan, H., Petropoulou, M., Spitkovsky, A., Sironi, L.: Secondary energiza- tion in compressing plasmoids during magnetic reconnection. The Astrophysical Journal912(1), 48 (2021) https://doi.org/10.3847/1538-4357/abedac
2021 doi
-
[45]
The Astrophysical Journal Letters954(2), 37 (2023) https://doi.org/10.3847/2041-8213/acf135
Li, X., Guo, F., Liu, Y.-H., Li, H.: A model for nonthermal particle acceleration in relativistic magnetic reconnection. The Astrophysical Journal Letters954(2), 37 (2023) https://doi.org/10.3847/2041-8213/acf135
2023 doi
-
[46]
Zhang, H., Sironi, L., Giannios, D., Petropoulou, M.: The origin of power-law spectra in relativistic magnetic reconnection (2023) 25
2023
-
[47]
Astronomy and Astrophysics262, 26–36 (1992)
Romanova, M.M., Lovelace, R.V.E.: Magnetic field, reconnection and parti- cle acceleration in extragalactic jets. Astronomy and Astrophysics262, 26–36 (1992)
1992
-
[48]
Monthly Notices of the Royal Astronomical Society: Letters395(1), 29–33 (2009) https://doi.org/10.1111/j.1745-3933.2009.00635.x
Giannios, D., Uzdensky, D.A., Begelman, M.C.: Fast tev variability in blazars: jets in a jet. Monthly Notices of the Royal Astronomical Society: Letters395(1), 29–33 (2009) https://doi.org/10.1111/j.1745-3933.2009.00635.x
2009
-
[49]
Monthly Notices of the Royal Astronomi- cal Society402(3), 1649–1656 (2010) https://doi.org/10.1111/j.1365-2966.2009
Giannios, D., Uzdensky, D.A., Begelman, M.C.: Fast TeV variability from misaligned minijets in the jet of m87. Monthly Notices of the Royal Astronomi- cal Society402(3), 1649–1656 (2010) https://doi.org/10.1111/j.1365-2966.2009. 16045.x
2010
-
[50]
Sironi, L., Petropoulou, M., Giannios, D.: Relativistic jets shine through shocks or magnetic reconnection? Monthly Notices of the Royal Astronomical Society 450(1), 183–191 (2015) https://doi.org/10.1093/mnras/stv641
2015 doi
-
[51]
Annual Review of Astronomy and Astrophysics57(1), 467–509 (2019) https://doi.org/10.1146/annurev-astro-081817-051948
Blandford, R., Meier, D., Readhead, A.: Relativistic jets from active galactic nuclei. Annual Review of Astronomy and Astrophysics57(1), 467–509 (2019) https://doi.org/10.1146/annurev-astro-081817-051948
2019 doi
-
[52]
Zhang, H., Li, X., Giannios, D., Guo, F., Liu, Y.-H., Dong, L.: Radiation and Polarization Signatures from Magnetic Reconnection in Relativistic Jets. I. A Systematic Study. Astrophysical Journal901(2), 149 (2020) https://doi.org/10. 3847/1538-4357/abb1b0 arXiv:2008.09444 [ast...
2020 arXiv
-
[53]
Space Sci Rev173, 521–533 (2012) https://doi.org/10.1007/s11214-012-9931-z
Hoshino, M., Lyubarsky, Y.: Relativistic reconnection and particle acceleration. Space Sci Rev173, 521–533 (2012) https://doi.org/10.1007/s11214-012-9931-z
2012 doi
-
[54]
Space Science Reviews 191(1-4), 545–573 (2015) https://doi.org/10.1007/s11214-014-0132-9
Kagan, D., Sironi, L., Cerutti, B., Giannios, D.: Relativistic magnetic reconnec- tion in pair plasmas and its astrophysical applications. Space Science Reviews 191(1-4), 545–573 (2015) https://doi.org/10.1007/s11214-014-0132-9
2015 doi
-
[55]
Physics of Plas- mas27(8), 080501 (2020) https://doi.org/10.1063/5.0012094 arXiv:2006.15288 [astro-ph.HE]
Guo, F., Liu, Y.-H., Li, X., Li, H., Daughton, W., Kilian, P.: Recent progress on particle acceleration and reconnection physics during magnetic reconnection in the magnetically-dominated relativistic regime. Physics of Plas- mas27(8), 080501 (2020) https://doi.org/10.1063/5.0...
2020 arXiv
-
[57]
Astrophysical Journal884(1), 57 (2019) https://doi.org/10.3847/1538-4357/ab3f2e arXiv:1908.05866 [astro-ph.HE] 26
Ball, D., Sironi, L., ¨Ozel, F.: The Mechanism of Electron Injection and Accelera- tion in Transrelativistic Reconnection. Astrophysical Journal884(1), 57 (2019) https://doi.org/10.3847/1538-4357/ab3f2e arXiv:1908.05866 [astro-ph.HE] 26
2019 arXiv
-
[58]
ApJ899(151), 15 (2020) https://doi.org/ 10.3847/1538-4357/aba1e9
Kilian, P., Li, X., Guo, F., Zhang, Q. ApJ899(151), 15 (2020) https://doi.org/ 10.3847/1538-4357/aba1e9
2020 doi
-
[59]
Journal of Plasma Physics87(6) (2021) https://doi.org/10.1017/ s0022377821001185
Werner, G.R., Uzdensky, D.A.: Reconnection and particle acceleration in three- dimensional current sheet evolution in moderately magnetized astrophysical pair plasma. Journal of Plasma Physics87(6) (2021) https://doi.org/10.1017/ s0022377821001185
2021
-
[60]
Nature443, 553 (2006) https: //doi.org/10.1038/nature05116
Drake, J.F., Swisdak, M., Che, H., Shay, M.A. Nature443, 553 (2006) https: //doi.org/10.1038/nature05116
2006 doi
-
[61]
Astrophysical Journal714(1), 915–926 (2010) https://doi.org/10.1088/0004-637X/714/1/915 arXiv:1004.1154 [astro- ph.SR]
Oka, M., Phan, T.-D., Krucker, S., Fujimoto, M., Shinohara, I.: Electron Accel- eration by Multi-Island Coalescence. Astrophysical Journal714(1), 915–926 (2010) https://doi.org/10.1088/0004-637X/714/1/915 arXiv:1004.1154 [astro- ph.SR]
2010 arXiv
-
[62]
Physics of Plasmas21, 092304 (2014) https://doi.org/10.1063/1.4894484
Dahlin, J.T., Drake, J.F., Swisdak, M.: The mechanisms of electron heating and acceleration during magnetic reconnection. Physics of Plasmas21, 092304 (2014) https://doi.org/10.1063/1.4894484
2014 doi
-
[63]
Physics of Plasmas 23(12), 120704 (2016) https://doi.org/10.1063/1.4972082
Dahlin, J.T., Drake, J.F., Swisdak, M.: Parallel electric fields are inefficient drivers of energetic electrons in magnetic reconnection. Physics of Plasmas 23(12), 120704 (2016) https://doi.org/10.1063/1.4972082
2016 doi
-
[64]
Physics of Plasmas24, 092110 (2017) https://doi.org/10.1063/1.4986211
Dahlin, J.T., Drake, J.F., Swisdak, M. Physics of Plasmas24, 092110 (2017) https://doi.org/10.1063/1.4986211
2017 doi
-
[65]
The Astrophysical Journal 811(2), 24 (2015) https://doi.org/10.1088/2041-8205/811/2/l24
Li, X., Guo, F., Li, H., Li, G.: Nonthermally dominated electron acceleration during magnetic reconnection in a low-beta plasma. The Astrophysical Journal 811(2), 24 (2015) https://doi.org/10.1088/2041-8205/811/2/l24
2015 doi
-
[66]
Astrophysical Journal843(1), 21 (2017) https: //doi.org/10.3847/1538-4357/aa745e
Li, X., Guo, F., Li, H., Li, G.: Particle Acceleration during Magnetic Recon- nection in a Low-beta Plasma. Astrophysical Journal843(1), 21 (2017) https: //doi.org/10.3847/1538-4357/aa745e
2017 doi
-
[69]
Physical Review Letters 27 114(6) (2015) https://doi.org/10.1103/physrevlett.114.061101
Hoshino, M.: Angular momentum transport and particle acceleration during magnetorotational instability in a kinetic accretion disk. Physical Review Letters 27 114(6) (2015) https://doi.org/10.1103/physrevlett.114.061101
2015 doi
-
[70]
The Astrophysical Journal900(2), 100 (2020) https://doi.org/10.3847/1538-4357/ababab
Ripperda, B., Bacchini, F., Philippov, A.A.: Magnetic reconnection and hot spot formation in black hole accretion disks. The Astrophysical Journal900(2), 100 (2020) https://doi.org/10.3847/1538-4357/ababab
2020 doi
-
[71]
Monthly Notices of the Royal Astronomical Society513(3), 4267–4277 (2022) https://doi.org/10.1093/mnras/stac1118
Nathanail, A., Mpisketzis, V., Porth, O., Fromm, C.M., Rezzolla, L.: Mag- netic reconnection and plasmoid formation in three-dimensional accretion flows around black holes. Monthly Notices of the Royal Astronomical Society513(3), 4267–4277 (2022) https://doi.org/10.1093/mnras/stac1118
2022 doi
-
[72]
Monthly Notices of the Royal Astronomical Society520(1), 1271–1284 (2023) https://doi.org/10.1093/mnras/stad176
Lin, X., Li, Y.-P., Yuan, F.: A ‘coronal-mass-ejection’ model for flares in sagit- tarius a*. Monthly Notices of the Royal Astronomical Society520(1), 1271–1284 (2023) https://doi.org/10.1093/mnras/stad176
2023 doi
-
[73]
Physical Review Letters85(22), 4656–4659 (2000) https://doi.org/10.1103/physrevlett
Chandran, B.D.G.: Scattering of energetic particles by anisotropic magneto- hydrodynamic turbulence with a goldreich-sridhar power spectrum. Physical Review Letters85(22), 4656–4659 (2000) https://doi.org/10.1103/physrevlett. 85.4656
2000 doi
-
[74]
Physical Review Letters118(5) (2017) https://doi.org/10.1103/physrevlett.118
Zhdankin, V., Werner, G.R., Uzdensky, D.A., Begelman, M.C.: Kinetic tur- bulence in relativistic plasma: From thermal bath to nonthermal continuum. Physical Review Letters118(5) (2017) https://doi.org/10.1103/physrevlett.118. 055103
2017 doi
-
[75]
Astrophysical Journal Letters867(1), 18 (2018) https://doi.org/10.3847/ 2041-8213/aae88c arXiv:1805.08754 [astro-ph.HE]
Zhdankin, V., Uzdensky, D.A., Werner, G.R., Begelman, M.C.: System-size Convergence of Nonthermal Particle Acceleration in Relativistic Plasma Turbu- lence. Astrophysical Journal Letters867(1), 18 (2018) https://doi.org/10.3847/ 2041-8213/aae88c arXiv:1805.08754 [astro-ph.HE]
2018 arXiv
-
[76]
Physical Review Letters122(5) (2019) https://doi.org/10.1103/physrevlett.122.055101
Zhdankin, V., Uzdensky, D.A., Werner, G.R., Begelman, M.C.: Electron and ion energization in relativistic plasma turbulence. Physical Review Letters122(5) (2019) https://doi.org/10.1103/physrevlett.122.055101
2019 doi
-
[77]
The Astrophysical Journal893(1), 7 (2020) https://doi.org/10.3847/2041-8213/ab8122
Wong, K., Zhdankin, V., Uzdensky, D.A., Werner, G.R., Begelman, M.C.: First- principles demonstration of diffusive-advective particle acceleration in kinetic simulations of relativistic plasma turbulence. The Astrophysical Journal893(1), 7 (2020) https://doi.org/10.3847/2041-8...
2020 doi
-
[78]
Nonideal Fields Solve the Injection Problem in Relativistic Reconnection
Guo, F., Li, X., French, O., Zhang, Q., Daughton, W., Liu, Y.-H., Matthaeus, W., Kilian, P., Johnson, G., Li, H.: Comment on “Nonideal Fields Solve the Injection Problem in Relativistic Reconnection”. Physical Review Let- ters130(18), 189501 (2023) https://doi.org/10.1103/Phys...
2023 arXiv
-
[79]
Astrophysical Journal Letters 952(1), 1 (2023) https://doi.org/10.3847/2041-8213/acdb60
Totorica, S.R., Zenitani, S., Matsukiyo, S., Machida, M., Sekiguchi, K., Bhat- tacharjee, A.: Exact Calculation of Nonideal Fields Demonstrates Their Dom- inance of Injection in Relativistic Reconnection. Astrophysical Journal Letters 952(1), 1 (2023) https://doi.org/10.3847/2...
2023 doi
-
[80]
https://arxiv
Singh, D., French, O., Guo, F., Li, X.: Low-energy Injection and Nonthermal Particle Acceleration in Relativistic Magnetic Turbulence (2024). https://arxiv. org/abs/2404.19181
2024 arXiv
-
[81]
In preparation for submission to the Astrophysical Journal (2024)
French, O., Werner, G.R., Uzdensky, D.A.: Particle Injection in 3D Relativis- tic Magnetic Reconnection. In preparation for submission to the Astrophysical Journal (2024)
2024
-
[82]
Zhang, Q., Guo, F., Daughton, W., Li, H., Le, A., Phan, T., Desai, M.: Multi- species Ion Acceleration in 3D Magnetic Reconnection with Hybrid-kinetic Simulations (2024)
2024
-
[83]
Astrophysical Journal866(1), 4 (2018) https://doi.org/10.3847/1538-4357/aae07b arXiv:1807.03427 [astro-ph.SR]
Li, X., Guo, F., Li, H., Li, S.: Large-scale Compression Acceleration during Mag- netic Reconnection in a Low-βPlasma. Astrophysical Journal866(1), 4 (2018) https://doi.org/10.3847/1538-4357/aae07b arXiv:1807.03427 [astro-ph.SR]
2018 arXiv
-
[84]
Physical Review Let- ters126(13), 135101 (2021) https://doi.org/10.1103/PhysRevLett.126.135101 arXiv:2011.01147 [physics.plasm-ph]
Arnold, H., Drake, J.F., Swisdak, M., Guo, F., Dahlin, J.T., Chen, B., Fleishman, G., Glesener, L., Kontar, E., Phan, T., Shen, C.: Electron Acceleration during Macroscale Magnetic Reconnection. Physical Review Let- ters126(13), 135101 (2021) https://doi.org/10.1103/PhysRevLet...
2021 arXiv
-
[85]
arXiv e-prints, 2404–12276 (2024) https://doi.org/10.48550/arXiv.2404.12276 arXiv:2404.12276 [astro-ph.HE]
Seo, J., Guo, F., Li, X., Li, H.: Proton Acceleration in Low-beta Magnetic Recon- nection with Energetic Particle Feedback. arXiv e-prints, 2404–12276 (2024) https://doi.org/10.48550/arXiv.2404.12276 arXiv:2404.12276 [astro-ph.HE]
-
[86]
Astronomy and Astrophysics441(3), 845–853 (2005) https://doi
de Gouveia dal Pino, E.M., Lazarian, A.: Production of the large scale super- luminal ejections of the microquasar GRS 1915+105 by violent magnetic reconnection. Astronomy and Astrophysics441(3), 845–853 (2005) https://doi. org/10.1051/0004-6361:20042590
2005 doi
-
[87]
Astrophysical Journal974(1), 28 (2024) https://doi.org/10.3847/1538-4357/ad6e80 arXiv:2408.10445 [astro-ph.SR]
Murtas, G., Li, X., Guo, F.: Compression Acceleration of Protons and Heavier Ions at the Heliospheric Current Sheet. Astrophysical Journal974(1), 28 (2024) https://doi.org/10.3847/1538-4357/ad6e80 arXiv:2408.10445 [astro-ph.SR]
2024 arXiv
-
[88]
Astrophysical Journal 974(1), 74 (2024) https://doi.org/10.3847/1538-4357/ad7131 arXiv:2407.10933 [physics.plasm-ph]
Yin, Z., Drake, J.F., Swisdak, M.: Simultaneous Proton and Electron Ener- gization during Macroscale Magnetic Reconnection. Astrophysical Journal 974(1), 74 (2024) https://doi.org/10.3847/1538-4357/ad7131 arXiv:2407.10933 [physics.plasm-ph]
2024 arXiv
-
[89]
Nonideal Fields Solve the 29 Injection Problem in Relativistic Reconnection
Guo, F., Li, X., French, O., Daughton, W., Matthaeus, W., Zhang, Q., Liu, Y.-H., Kilian, P., Johnson, G., Li, H.: Comment on “Nonideal Fields Solve the 29 Injection Problem in Relativistic Reconnection”. arXiv (2022). https://doi.org/ 10.48550/ARXIV.2208.03435 . https://arxiv....
-
[90]
The Astrophysical Journal586(1), 72–78 (2003) https://doi.org/10.1086/367640
Larrabee, D.A., Lovelace, R.V.E., Romanova, M.M.: Lepton acceleration by rel- ativistic collisionless magnetic reconnection. The Astrophysical Journal586(1), 72–78 (2003) https://doi.org/10.1086/367640
2003 doi
-
[91]
The Astrophysical Journal677(1), 530–544 (2008) https://doi
Zenitani, S., Hoshino, M.: The role of the guide field in relativistic pair plasma reconnection. The Astrophysical Journal677(1), 530–544 (2008) https://doi. org/10.1086/528708
2008 doi
-
[92]
The Astrophysical Jour- nal782(2), 104 (2014) https://doi.org/10.1088/0004-637x/782/2/104
Cerutti, B., Werner, G.R., Uzdensky, D.A., Begelman, M.C.: THREE- DIMENSIONAL RELATIVISTIC PAIR PLASMA RECONNECTION WITH RADIATIVE FEEDBACK IN THE CRAB NEBULA. The Astrophysical Jour- nal782(2), 104 (2014) https://doi.org/10.1088/0004-637x/782/2/104
2014 doi
-
[93]
Physical Review Let- ters127(18), 185101 (2021) https://doi.org/10.1103/PhysRevLett.127.185101 arXiv:2105.04521 [astro-ph.SR]
Zhang, Q., Guo, F., Daughton, W., Li, H., Li, X.: Efficient Nonther- mal Ion and Electron Acceleration Enabled by the Flux-Rope Kink Insta- bility in 3D Nonrelativistic Magnetic Reconnection. Physical Review Let- ters127(18), 185101 (2021) https://doi.org/10.1103/PhysRevLett.1...
2021 arXiv
-
[94]
Physics of Plasmas30(4) (2023) https://doi.org/10.1063/5.0139276
Majeski, S., Ji, H.: Super-fermi acceleration in multiscale MHD reconnection. Physics of Plasmas30(4) (2023) https://doi.org/10.1063/5.0139276
2023 doi
-
[95]
The Astro- physical Journal700, 16–20 (2009) https://doi.org/10.1088/0004-637X/700/1/ L16
Drake, J.F., Cassak, P.A., Shay, M.A., Swisdak, M., Quataert, E. The Astro- physical Journal700, 16–20 (2009) https://doi.org/10.1088/0004-637X/700/1/ L16
2009 doi
-
[96]
The Astrophysical Journal 899(1), 52 (2020) https://doi.org/10.3847/1538-4357/aba622
Sironi, L., Beloborodov, A.M.: Kinetic simulations of radiative magnetic recon- nection in the coronae of accreting black holes. The Astrophysical Journal 899(1), 52 (2020) https://doi.org/10.3847/1538-4357/aba622
2020 doi
-
[97]
Chernoglazov, A., Hakobyan, H., Philippov, A.A.: High-Energy Radiation and Ion Acceleration in Three-dimensional Relativistic Magnetic Reconnection with Strong Synchrotron Cooling (2023)
2023
-
[98]
https://arxiv.org/abs/2501.00979
Gupta, S., Sridhar, N., Sironi, L.: The Role of Electric Dominance for Particle Injection in Relativistic Reconnection (2025). https://arxiv.org/abs/2501.00979
2025 arXiv
-
[99]
Physics of Plasmas29(4) (2022) https://doi.org/10.1063/5.0086316
Hoshino, M.: Efficiency of nonthermal particle acceleration in magnetic recon- nection. Physics of Plasmas29(4) (2022) https://doi.org/10.1063/5.0086316
2022 doi
-
[100]
Physics of Plasmas29(5), 052904 30 (2022) https://doi.org/10.1063/5.0085647
Oka, M., Phan, T., Øieroset, M., Turner, D., Drake, J., Li, X., Fuselier, S., Ger- shman, D., Giles, B., Ergun, R., Torbert, R., Wei, H., Strangeway, R., Russell, C., Burch, J.: Electron energization and thermal to non- thermal energy parti- tion during earth’s magnetotail rec...
2022 doi
-
[101]
Physics of Plasmas31(5), 052901 (2024) https://doi.org/10.1063/5.0201845 arXiv:2404.15662 [astro-ph.HE]
Hoshino, M.: A hard energy spectrum in 3D guide-field magnetic reconnection. Physics of Plasmas31(5), 052901 (2024) https://doi.org/10.1063/5.0201845 arXiv:2404.15662 [astro-ph.HE]
2024 arXiv
-
[102]
Geophysical Research Letters49(9), 96986 (2022) https://doi.org/10.1029/2021GL09698610.1002/essoar.10508706.1
Phan, T.D., Verniero, J.L., Larson, D., Lavraud, B., Drake, J.F., Øieroset, M., Eastwood, J.P., Bale, S.D., Livi, R., Halekas, J.S., Whittlesey, P.L., Rahmati, A., Stansby, D., Pulupa, M., MacDowall, R.J., Szabo, P.A., Koval, A., Desai, M., Fuselier, S.A., Velli, M., Hesse, M....
2022
-
[103]
The Astrophysical Journal927(1), 62 (2022) https://doi.org/10
Desai, M.I., Mitchell, D.G., McComas, D.J., Drake, J.F., Phan, T., Szalay, J.R., Roelof, E.C., Giacalone, J., Hill, M.E., Christian, E.R., Schwadron, N.A., McNutt, R.L., Wiedenbeck, M.E., Joyce, C., Cohen, C.M.S., Davis, A.J., Krim- igis, S.M., Leske, R.A., Matthaeus, W.H., Ma...
2022
-
[104]
Astrophysical Journal898(2), 154 (2020) https://doi.org/10.3847/1538-4357/ ab9ab6
Ergun, R.E., Ahmadi, N., Kromyda, L., Schwartz, S.J., Chasapis, A., Hoili- joki, S., Wilder, F.D., Stawarz, J.E., Goodrich, K.A., Turner, D.L., Cohen, I.J., Bingham, S.T., Holmes, J.C., Nakamura, R., Pucci, F., Torbert, R.B., Burch, J.L., Lindqvist, P.-A., Strangeway, R.J., Le...
2020 doi
-
[105]
Astrophysical Journal932(2), 92 (2022) https://doi.org/10.3847/ 1538-4357/ac6efe arXiv:2205.04946 [astro-ph.SR] 31 Fig
Li, X., Guo, F., Chen, B., Shen, C., Glesener, L.: Modeling Electron Accelera- tion and Transport in the Early Impulsive Phase of the 2017 September 10th Solar Flare. Astrophysical Journal932(2), 92 (2022) https://doi.org/10.3847/ 1538-4357/ac6efe arXiv:2205.04946 [astro-ph.SR...
2022 arXiv
Reviewed August 15, 2026 · model on record in the stance chip above.
Discussion (0). Continue with ORCID to comment.