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Strangelets: Mass Formula

The basic idea that a new form of matter, so-called strange quark matter, might exist and be stable against strong decay (or possibly even absolutely stable) has been suggested in Refs. [2, 3, 7]. The discovery of strange quark matter, or the determination of significant upper limits for its production rate, is a major goal of the proposed experiment. The ``new'' matter consists of multi quark states containing u, d, and s quarks in a single ``bag.'' In essence, the strangeness degree of freedom allows more quarks to occupy low lying levels than is possible with two flavors. This leads to the possibility that an assembly of baryon number, A, might be metastable or even stable when all of the quarks are in a single bag. This is in contrast to the case of ordinary nuclei where the quarks of a large A system are (mostly!) organized into 3 quark, color-neutral bags (the neutrons and protons) which interact with one another by meson exchange forces.

A mass formula of Bethe-Weizacker type for strangelets was developed in Ref. [23]. The energy E(A,Y,Z) of a strangelet of baryon number A, hypercharge Y=A+S (S = strangeness) and electric charge Z assumes the form

displaymath2109

The two parameters of the theory are the energy per baryon tex2html_wrap_inline2111 in bulk matter (large A) and the strange quark mass tex2html_wrap_inline2007 . The most stable strangelets have (Y,Z) close to ( tex2html_wrap_inline2121 , tex2html_wrap_inline2123 ). The quantities of interest here, namely the regions of tex2html_wrap_inline2125 where the system is stable with respect to weak and strong neutron emission, are much more sensitive to tex2html_wrap_inline2111 than tex2html_wrap_inline2007 . The strangelet surface tension, tex2html_wrap_inline2131 , radius parameter tex2html_wrap_inline2133 , as well as the parameters tex2html_wrap_inline2135 , tex2html_wrap_inline2121 , tex2html_wrap_inline2139 , tex2html_wrap_inline2123 of the above Taylor expansion can all be expressed in terms of tex2html_wrap_inline2007 and an angle tex2html_wrap_inline2145 defined by

displaymath2147

In particular,

displaymath2149

displaymath2151

Typically, the strangelet density tex2html_wrap_inline2153 is of order twice that of non-strange nuclear matter. In weak or strong neutron emission from strangelets, respectively, the energy releases tex2html_wrap_inline2155 are given by

displaymath2157

displaymath2159

The qualitative features of strangelet stability, as a function of y=Y/A and A, for fixed tex2html_wrap_inline2165  MeV, tex2html_wrap_inline2167  MeV/c tex2html_wrap_inline2169 and tex2html_wrap_inline2171 , are shown in Fig. gif, taken from Berger and Jaffe [23]. For A=15, typical stability regions in the (Z,Y) plane are indicated in Fig. gif, from Ref. [4]. As tex2html_wrap_inline2111 increases towards the neutron mass tex2html_wrap_inline2179 , the region of strong neutron decay marches to the left in Fig. gif, and intersects the weak decay region, which marches to the right. If there is a gap between the weak and strong decay regions, E864 would have the best chance of finding a stable strangelet with tex2html_wrap_inline2181 and tex2html_wrap_inline2183 , in the vicinity of the dot in Fig. gif. At AGS energies, since the amount of strangeness produced is limited, the region of stability for tex2html_wrap_inline2185 is probably not accessible. For tex2html_wrap_inline2187 , the value of tex2html_wrap_inline2189 is given roughly by

displaymath2191

For tex2html_wrap_inline2167 MeV, the variation of tex2html_wrap_inline2189 with tex2html_wrap_inline2111 is displayed in Table gif.

  
Figure: Strangelet stability as a function of Y and A for fixed tex2html_wrap_inline2165  MeV, tex2html_wrap_inline2167  MeV/c tex2html_wrap_inline2169 , and tex2html_wrap_inline2171 . From Ref. [23].

  
Figure: Stability regions in the (Z,Y) plane for an A=15 strangelet. From Ref. [23].

   table209
Table: The variation of tex2html_wrap_inline2189 with tex2html_wrap_inline2111 for tex2html_wrap_inline2167  MeV.

Note that tex2html_wrap_inline2145 , tex2html_wrap_inline2121 , tex2html_wrap_inline2133 and tex2html_wrap_inline2131 vary only weakly with changes in tex2html_wrap_inline2111 , whereas tex2html_wrap_inline2189 and the associated strangeness value tex2html_wrap_inline2259 are very sensitive to tex2html_wrap_inline2111 .

There is clearly a limit to the amount of strangeness and baryon number that we can assemble in a bound strangelet, starting with the hadronic soup resulting from a central Au-Au collision. The coalescence estimates presented later, although perhaps somewhat conservative, suggest that composite strange clusters with tex2html_wrap_inline2263 might be formed with measurable rates in E864. Thus if tex2html_wrap_inline2111 is too large, we cannot fabricate a cluster with tex2html_wrap_inline2267 . Inspection of Table gif reveals that if tex2html_wrap_inline2269 MeV, we are in the domain of sensitivity of E864. Viewed in the context of an assumed Bethe-Weizacker mass formula, the absence of a strangelet signal in E864 could be translated into a constraint on the volume term tex2html_wrap_inline2111 .

The calculations based on the MIT Bag Model, which yield a Bethe-Weizacker mass formula, are suggestive but clearly are not definitive predictions. Since this approach is essentially a Taylor series in tex2html_wrap_inline2273 , it is not reliable for small A. In particular, it is unclear at what minimum value of A stable strangelets tex2html_wrap_inline2279 occur. Farhi and Jaffe [7] have done explicit quark shell model calculations for tex2html_wrap_inline2281 , finding no stable strangelets (the H-dibaryon is a possible exception, treated explicitly later). That perturbative calculation was based on one-gluon exchange; multi-quark states with a high degree of symmetry may become stable because of non-perturbative effects [24]. Thus one should properly regard the possible existence of strange quark matter as a question to be resolved by experiment.




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Next: Production of Strangelets in Up: Physics Goals Previous: Multi-Strange Clusters

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Tue Jan 21 17:29:21 EST 1997