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High-energy Neutrino Predictions for T Coronae Borealis: Probing Particle Acceleration in Novae

  • Authors: Prantik Sarmah, Sovan Chakraborty, Xilu Wang

Prantik Sarmah et al 2026 The Astrophysical Journal Letters 1001 .

  • Provider: AAS Journals

Caption: Figure 3.

Muon neutrino flux from MR model (shown in green) compared with that from the ES model (shown in blue) for T CrB. The green curves depict the fluxes for T CrB (solid) and RS Oph (dotted) corresponding to the benchmark parameters in Table 2, whereas the green band shows the uncertainties due to parameter variations. The sensitivities of IceCube and KM3NeT are same as in the Figure 2.

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