TYPE IA SUPERNOVA COUNTS AT HIGH-Z - SIGNATURES OF COSMOLOGICAL MODELS AND PROGENITORS

Determination of the rates at which Type Ia supernovae (SNe Ia) occur in the early universe can give signatures of the time spent by the bin ary progenitor systems to reach explosion and of the geometry of the u niverse. Observations made within the Supernova Cosmology Project are already providing the first numbers. Here it is shown that, for any as sumed SNe Ia progenitor, SNe Ia counts up to m(R) similar or equal to 23-26 are useful tests of the SNe Ia progenitor systems and cosmologic al tracers of a possible nonzero value of the cosmological constant, L ambda. The SNe Ia counts at high redshifts compare differently with th ose at lower redshifts depending on the cosmological model. A flat, Om ega(Lambda)-dominated universe would show a more significant increase of the SNe Ia counts at z similar to 1 than a flat, Omega(M) = 1 unive rse. Here we consider three sorts of universes: a flat universe with H -0 = 65 km s(-1) Mpc(-1), Omega(M) = 1.0, Omega(Lambda) = 0.0; an open universe with H-0 = 65 km s(-1) Mpc(-1), Omega(M) = 0.3, Omega(Lambda ) = 0.0; and a hat, Lambda-dominated universe with H-0 = 65 km s(-1) M pc(-1), Omega(M) = 0.3, Omega(Lambda) = 0.7. On the other hand, the SN e Ia counts from one class of binary progenitors (double-degenerate sy stems) should not increase steeply in the z = 0-1 range, contrary to w hat should be seen for other binary progenitors. A measurement of the SNe Ia counts up to z similar to 1 is within reach of ongoing SNe Ia s earches at high redshifts.