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• W2914772005 startingPage "L141" @default.
• W2914772005 abstract "A possibility of generating a population of cosmic-ray particles accelerated in supernovae typeIa (SNIa) remnants in the intracluster medium (ICM) is discussed. The presently constrained host-less SNIa rates in the clusters are found to be sufficient to fill a few hundred kpc region with cosmic-ray electrons within their typical synchrotron life-time of 100 Myr. The SNIa have already been considered potential sources of excess Fe abundance in cool-core clusters, distributed heating and turbulence in ICM. A good fraction of total radio power from mini-halos can be sourced from the SNIa energy deposited in the ICM with required energy conversion efficiency <1 per cent. The radio power estimated from low Mach number shock acceleration in SNIa remnants is consistent with the observations within the uncertainties in the estimates. Some observational properties of the radio mini-halos are broadly consistent with the SNIa scenario. It is also speculated that radio powers and possibly detections of mini-halos are linked to star formation and merger histories of the clusters." @default.
• W2914772005 created "2019-02-21" @default.
• W2914772005 creator A5052275053 @default.
• W2914772005 date "2019-02-14" @default.
• W2914772005 modified "2023-09-28" @default.
• W2914772005 title "Role of intracluster supernovae in radio mini-haloes in galaxy clusters" @default.
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• W2914772005 doi "https://doi.org/10.1093/mnrasl/slz020" @default.
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