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A simultaneous description of non-strange nuclei, hypernuclei andmultiply-strange nuclear systems is provided by a single mass formula which isshown to be useful for estimating binding energies of nuclear systems over awide mass range, including the light mass nuclei. It not only provides a goodfit to the existing experimental data on hyperon-separation energies but alsoreproduces results of the relativistic mean field (RMF) calculations. Inaddition, it can provide the Lambda($\Lambda$), Cascade-0($\Xi^0$) andCascade-minus ($\Xi^-$) drip lines. The existence of a range of boundpure-hyperonic systems without any neutron and proton is suggested among which$6\Lambda$, $9\Xi^0\Xi^0$, $10\Xi^-\Xi^-$, $1\Lambda7\Xi^0$, $1\Lambda 8\Xi^-$,$1\Xi^09 \Xi^-$, $1\Xi^- 8\Xi^0$ and $2\Lambda+3\Xi^0+3\Xi^-$ represent thelightest species. In agreement with the RMF predictions, this generalized massformula also predicts the nucleus $_{2\Xi^0 2\Lambda}{^8He}$ to be bound. Anexotic $_{2\Xi^0 2\Xi^- 2\Lambda}{^{10}n}$ nucleus is also found to be bound.This new mass formula can be used in astrophysics for strange stellar objects,as well as in high energy physics for estimating the strangeness productionyield in nucleus-nucleus or, nucleon-nucleon collisions.

Generalised mass formula for non-strange, strange and multiply-strange nuclear systems