“…Depending on the actual temperatures achieved during collapse, different excitations become dominant in the compressed gas, so that ''thermal emission'' can refer to a large variety of different processes. As temperatures increase from several hundred to many thousand kelvin, those processes can be, among others, molecular recombination (Saksena and Nyborg, 1970), collision-induced emission (Frommhold and Atchley, 1994), molecular emission (Didenko et al, 2000b), excimers (Hammer and Frommhold, 2001), atomic recombination (Hilgenfeldt et al, 1999b), radiative attachment of ions (Hammer and Frommhold, 2001), neutral and ion bremsstrahlung (Moss et al, 1997;Xu et al, 1998;Hilgenfeldt et al, 1999b), or emission from confined electrons in voids (Bernstein and Zakin, 1995). The uncertainty about the precise temperatures of SBSL bubbles (see Sec.…”