Goldhaber also demonstrated how a "time-dilation" factor
related to the expansion of the universe serves to refute alternative proposals as an
explanation of the high redshifts seen in distant type Ia supernovae.
The Supernova Cosmology Project is an international collaboration headed by Berkeley
Lab astrophysicist Saul Perlmutter. This collaboration shared the Science award with
another international collaboration, the High-z Supernova Search Team led by Brian Schmidt
of Australia's Mount Stromlo and Siding Spring Observatories, for the discovery that the
universe is expanding at an accelerating rate. The discovery was made through the
observation of type Ia supernovae.
Because all type Ia supernovae have the same intrinsic light curves (a measurement of
the rise and fall of their light output), they can act as clocks over cosmological
distances. Having traveled a longer time to get here, light from more distant supernovae
shows a higher redshift (a shift in spectral lines to longer wavelengths) than light from
relatively nearby supernovae.
Redshifts in the spectral lines of distant stars were first observed in 1926 by Edwin
Hubble, who attributed the phenomenon to an expansion of the universe. Since then, rival
theories have been submitted to explain redshifts without the need for an expanding
universe.
In 1995 Goldhaber showed that for a few type Ia supernovae the observation of a
time-dilation factor could serve as a direct test of cosmological expansion. Since then,
he and his colleagues have measured the light curves of 35 high-redshift supernovae from
the more than 80 discovered by the Supernova Cosmology Project collaboration. The data for
each of these 35 supernovae were shown to share more than 1400 experimental points along a
common light curve when a cosmological expansion factor was taken into account.
"In an expanding universe, the light curve spread should behave the same as the
redshift of spectral features," says Goldhaber. "We have concluded that our data
are in agreement with this behavior."
Without factoring in cosmological expansion, the light curves of the individual
supernovae could not be combined. Goldhaber calls this a "strong argument"
against the "tired light" theory, in which the observed redshift in Type Ia
supernovae is attributed to the loss of energy by photons as they travel across the
universe.
"A mechanism that degrades photon energy, such as tired light, would not affect
the spacing between light emitted at different epochs of the light curve, and hence would
not affect its shape," Goldhaber says. "Our findings can only be explained by
the expansion of the universe."