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gwem_resampling [2022/10/31 09:43]
theoastro 		gwem_resampling [2023/01/04 11:46] (current)
theoastro
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 ===== GW-EM Resampling ===== ===== GW-EM Resampling =====
  
-In NMMA, it is possible to use the results from GRB, kilonova and GRB afterglow inferences to get estimates on the binary properties. This is based on phenomenological relations, i.e., via fits based on numerical-relativity relations. +In NMMA, it is possible to use the results from GW, kilonova and GRB afterglow inferences to get estimates on the binary properties. This is based on phenomenological relations, i.e., via fits based on numerical-relativity relations. 
 The dynamical ejecta mass,  \(M_{ej}^{dyn}\), is connected to the binary properties through quasi-universal relations, see [[https://arxiv.org/pdf/2205.08513.pdf|Pang et al. 2022]]. The dynamical ejecta mass,  \(M_{ej}^{dyn}\), is connected to the binary properties through quasi-universal relations, see [[https://arxiv.org/pdf/2205.08513.pdf|Pang et al. 2022]].
  
Last modified: le 2022/10/31 09:43

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