Abstract
The influence of modification of the effective mass of weakly interacting light boson (WILB) present in the compact hyperonic stars are investigated within the framework of the extended relativistic mean field model. It is found that the bulk properties of the hyperonic stars are compatible with the provided recent observational constraints, if the presence of the WILBs with appropriate effective mass is considered.
| Original language | English |
|---|---|
| Pages (from-to) | 501-504 |
| Number of pages | 4 |
| Journal | Few-Body Systems |
| Volume | 54 |
| Issue number | 1-4 |
| DOIs | |
| Publication status | Published - Mar 2013 |