Power-law index and cutoff of particles accelerated by reconnection · revision history
Revision 2
Accepted · core change · record
Changes against revision 1:
- Title
- Power-law index and cutoff of particles accelerated by reconnection
- Plain
- Reconnection in strongly magnetized astrophysical plasmas makes particles with a power-law energy distribution, few particles at high energy but many more than a thermal gas has. How steep that power law is and how high it extends is not settled.
- Precise · changed · core
- Revision 1: For relativistic pair-plasma or electron-ion reconnection with magnetization $\sigma = B^2/(4 \pi w)$ ($w$ = relativistic enthalpy density) from 1 to 1e3, determine the index $p$ of dN/dgamma ~ gamma^-p and the high-energy cutoff $\gamma_{\max}$ as functions of $\sigma$, guide field and system size $L/d_e$ in 3D, in the limit $L/d_e$ going to infinity. An answer is $p(\sigma, B_g)$ and the scaling of $\gamma_{\max}$ with $L$, converged in system size.
- Revision 2: For relativistic pair-plasma or electron-ion reconnection with magnetization $\sigma = B^2/(4 \pi w)$ ($w$ = relativistic enthalpy density) from 1 to $10^{3}$, determine the index $p$ of $dN/dgamma \sim \gamma^{-p}$ and the high-energy cutoff $\gamma_{\max}$ as functions of $\sigma$, guide field and system size $L/d_e$ in 3D, in the limit $L/d_e$ going to infinity. An answer is $p(\sigma, B_g)$ and the scaling of $\gamma_{\max}$ with $L$, converged in system size.
- Settled by · changed · core
- Revision 1: 3D particle-in-cell simulations converged in system size, with an analytic acceleration model reproducing $p\ \text{and}\ \gamma_{\mathrm{max}}$.
- Revision 2: 3D particle-in-cell simulations converged in system size, with an analytic acceleration model reproducing $p\ \text{and}\ \gamma_{\max}$.
- Kind
- well-posed
- Answer type
- value
- References
- (empty)
- Literature status
- contested
- Status note
- Particle-in-cell work through 2025 finds $p$ approaching $1 \text{ to } 2$ at $\sigma$ much larger than 1, but convergence with system size and the role of 3D effects are disputed.
- Posed since
- (empty)
Decisions
- Accept · 2026-10-15 · record