Nuclear Components

The electron spectrum which CALET could measure for case of annihilation of a Kaluza-Klein dark matter population added to the galactic background spectrum (dashed line).

Figure 1. The electron spectrum which CALET
could measure for case of annihilation of a Kaluza-Klein
dark matter population added to the galactic
background spectrum (dashed line).

Since CALET has excellent e-p separation, measuring the proton spectrum to very high energy will be straight-forward. The nuclear components are particularly important since they are the other side of the cosmic ray puzzle. One can change the source or propagation parameters to fit e.g. the total electrons, but such changes must be consistent with the nuclear spectra if, as most believe, the same sources accelerated both hadrons and leptons. The challenge here is energy resolution. In a calorimetric instrument, the leakage of energy from the bottom is much larger for a hadronic cascade than for an electromagnetic shower, and this limits the possible energy resolution for nuclei. Clearly, the deeper the calorimeter the better.

With the charge resolution provided by the scintillating fibers in the IMC plus the charge detector at the top, CALET will achieve another major objective -- measuring the Spectra of the Nuclear Component to the highest possible energies, limited only by exposure. The expected results for Hydrogen and Helium are illustrated in Figure 16. At high energy, the balloon data from ATIC [28] and CREAM [29] have verified that the spectra of H and He are different in the very high energy region and that neither are well represented by simple power laws. Rather, the spectra seem to be evolving, becoming harder with increasing energy. Whether this is a source/acceleration effect or is connected to particle transport in the galaxy remains an open question. CALET will have both the statistical precision and the energy reach to trace out any changes and/or major structures in these spectra.

CALET measurements of the primary heavy nuclei super-posed on existing data. The flux values are multiplied by E<sup>2.5</sup>.

Figure 2. CALET measurements of the primary heavy nuclei super-posed
on existing data. The flux values are multiplied by E^2.5.

With the charge resolution anticipated for CALET, the instrument will also be able to measure the spectra of the major primary elements to the iron peak. In this area there is some disagreement among the balloon experiments with some showing a trend to harder spectra with increasing energy while other experiments find a pure power law over the entire energy range [29,30]. As illustrated in Figure 17, CALET data will be able to resolve such effects and extend the available results to considerably higher energies.