Experimental investigation of an electronegative cylindrical capacitively coupled geometrically asymmetric plasma discharge with an axisymmetric magnetic field

We investigate the discharge characteristics of a low-pressure geometrically asymmetric cylindrical capacitively coupled plasma discharge with an axisymmetric magnetic field generating an EXB drift in the azimuthal direction. Vital discharge parameters, including electron density, electron temperature, DC self-bias, and Electron Energy distribution function (EEDF), are studied experimentally for varying magnetic field strength (B). A transition in the discharge asymmetry is observed along with a range of magnetic fields where the discharge is highly efficient with lower electron temperature. Outside this range of magnetic field, the plasma density drops, followed by an increase in the electron temperature. The observed behavior is attributed to the transition from geometrical asymmetry to magnetic field-associated symmetry due to reduced radial losses and plasma confinement in the peripheral region. In this region, the DC self-bias increases almost linearly from a large negative value to nearly zero, i.e., the discharge becomes symmetric. The EEDF undergoes a transition from bi-Maxwellian for unmagnetized to Maxwellian at intermediate B and finally becomes a weakly bi-Maxwellian at higher values of B. The above transitions present a novel way to independently control the ion energy and ion flux in a cylindrical CCP system using an axisymmetric magnetic field with an enhanced plasma density and lower electron temperature operation that is beneficial for plasma processing applications.

Discharge characteristics of a low-pressure geometrically asymmetric cylindrical capacitively coupled plasma with an axisymmetric magnetic field

We study the bound orbit conditions for equatorial and eccentric orbits around a Kerr black hole both in the parameter space ( E , L , a ) representing the energy, angular mo-mentum of the test particle, and spin of the black hole, and also ( e , µ , a ) space rep- resenting the eccentricity, inverse-latus rectum of the orbit, and spin. We apply these conditions and implement the relativistic precession (RP) model to M82X-1, which is an Intermediate-mass black hole (IMBH) system, where two high-frequency Quasi-Periodic Oscillations (HFQPOs) and a low-frequency QPO were simultaneously observed. As- suming that the QPO frequencies can also be generated by equatorial and eccentric trajectories, we calculate the probability distributions to infer e , a , and periastron dis- tance, r p , of the orbit giving rise to simultaneous QPOs. We ﬁnd that an eccentric orbit solution is possible in the region between innermost stable circular orbit (ISCO) and the marginally bound circular orbit (MBCO) for e = 0 . 2768 +0 . 0657 − 0 . 0451 , a = 0 . 2897 ± 0 . 0087, and r p = 4 . 6164 +0 . 0694 − 0 . 1259 .

https://doi.org/10.1142/9789811258251_0020

Eccentric equatorial trajectories around a Kerr black hole as a QPO model for M82X-1

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Discharge characteristics of a low-pressure geometrically asymmetric cylindrical capacitively coupled plasma with an axisymmetric magnetic field

Eccentric equatorial trajectories around a Kerr black hole as a QPO model for M82X-1