Table 1.
Properties of the different cases considered in the present study for calculating emission from the radio lobe.
| Run ID | DSA | STA | Turbulent decay | α | Remarks |
|---|---|---|---|---|---|
| Case (a) | YES | NO | NO | 0 | Energy spectrum exhibits power law with exponential cutoff; PDF of γavg shows power law; SED shows transient peaks. |
| Case (b) | YES | YES | YES | 104 | Individual macro-particle energy spectrum exhibits curvature; γmax PDF indicates accumulation of particles around 104; γavg PDF exhibits low-energy cutoff. Peak radiation from synthetic SED is 1010 Hz through synchrotron and 1019 Hz via IC-CMB. |
| Case (c) | YES | YES | YES | 105 | Individual macro-particle energy spectrum exhibits curvature. γmax PDF shows particle accumulation around 105; γavg PDF provides evidence of low-energy cutoff. Synthetic SED peak at 1013 Hz through syncrotron and 1021 Hz via IC-CMB. |
| Case (d) | YES | YES | NO | 104 | Individual macro-particle energy spectrum exhibits steady ultra-relativistic Maxwellian structure peaking at γ ≈ 104. |
| Case (e) | YES | YES | NO | 105 | Individual macro-particle energy spectrum exhibits steady ultra-relativistic Maxwellian structure peaking at γ ≈ 105. |
Notes. Column 1 gives the case labels for further reference. Columns 2–4 represent the presence or absence of DSA, STA, and turbulent decay effects on the emission runs. Column 5 gives the value of the free parameter α (Eq. (14)) chosen for different runs. The last column describes the results for each of the cases.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.