The Mass cut - The relation between 44Ti and 56Ni in supenovae remnants

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The discussion centers on the significance of the mass cut in core-collapse supernovae, specifically the ratio of 44Ti to 56Ni. The 44Ti isotope is utilized to trace the distribution of ejected material, as it is located further from the neutron star remnant. The inclusion of 56Ni is crucial because it plays a key role in the energy generation and light curve of supernovae, providing insights into nucleosynthesis processes. Understanding the relationship between these isotopes helps in mapping the ejecta and analyzing the remnants of supernovae. The referenced paper may offer additional insights into the nuclear processes involved.
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Would it be possible if you would help me with a quick question, (as none of the staff here, or postgraduates can answer this question)?

My group are designing a gamma ray telescope to look at nucleosynthesis in Supernovae. We have found a thing called the 'mass cut' (the separation between ejected material and the neutron-star remnant of a core-collapse supernova) which is defined as the ratio between 44Ti/56Ni.

I am basically wondering why you use such elements. It is known that 44Ti can be used to map the ejecta (as it will be far from the neutron star in the middle) from supenovae, but why would you use 56Ni?

Regards,

Paul
 
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