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A Study of Magnetized Plasma Turbulence in the Nonrelativistic and Relativistic Regimes.
A Study of Magnetized Plasma Turbulence in the Nonrelativistic and Relativistic Regimes.
- 자료유형
- 학위논문
- Control Number
- 0017161661
- International Standard Book Number
- 9798382580050
- Dewey Decimal Classification Number
- 530
- Main Entry-Personal Name
- Vega, Cristian S.
- Publication, Distribution, etc. (Imprint
- [S.l.] : The University of Wisconsin - Madison., 2024
- Publication, Distribution, etc. (Imprint
- Ann Arbor : ProQuest Dissertations & Theses, 2024
- Physical Description
- 167 p.
- General Note
- Source: Dissertations Abstracts International, Volume: 85-11, Section: B.
- General Note
- Advisor: Boldyrev, Stanislav.
- Dissertation Note
- Thesis (Ph.D.)--The University of Wisconsin - Madison, 2024.
- Summary, Etc.
- 요약Turbulence is ubiquitous in space and astrophysical plasmas and is believed to play an important role in particle heating and nonthermal acceleration. These plasmas are commonly threaded by an external magnetic field imposed by the object they surround (e.g., planet, star), making magnetized plasma turbulence a problem of significant interest. In this thesis, we use numerical simulations to study two relatively unexplored regimes of magnetized plasma turbulence, viz., the sub-electron inertial scale in nonrelativistic low electron beta plasmas and both the magnetohydrodynamic and kinetic scales in relativistically hot plasmas. Phenomenology is used to model the energy distribution of turbulent fluctuations and particles.In the nonrelativistic regime studied, energy dissipation is seen to be strongly intermittent, concentrating on electron-scale current sheets. A few of these current sheets exhibit signatures of electron-only reconnection.The particle energy probability density function in the relativistic regime displays a nonthermal tail of ultrarelativistic particles that goes from power-law-like to log-normal as the guide field is increased. We propose that this can be understood in terms of the acceleration mechanism that dominates in each case. Also noteworthy is the observed intermittency in the spatial distribution of ultrarelativistic particles.
- Subject Added Entry-Topical Term
- Plasma physics.
- Subject Added Entry-Topical Term
- Astrophysics.
- Subject Added Entry-Topical Term
- Theoretical physics.
- Index Term-Uncontrolled
- High-energy astrophysics
- Index Term-Uncontrolled
- Magnetic reconnection
- Index Term-Uncontrolled
- Magnetized plasma turbulence
- Index Term-Uncontrolled
- Relativistic plasmas
- Index Term-Uncontrolled
- Planet
- Added Entry-Corporate Name
- The University of Wisconsin - Madison Physics
- Host Item Entry
- Dissertations Abstracts International. 85-11B.
- Electronic Location and Access
- 로그인을 한후 보실 수 있는 자료입니다.
- Control Number
- joongbu:657122