The comparison of near and far supernovae by the High-Z Supernova Search Team (Riess et al. 1998) and by the Supernova Cosmology Project team (Perlmutter et al. 1999) revealed the surprising transition of Universe’s expansion from deceleration to acceleration.
The research teams found that remote supernovae were 10% to 25% dimmer and therefore further away than expected as compared to the nearby local supernovae.
Using type Ia supernovae, the research teams put forward “the first conclusive evidence for cosmic deceleration that preceded the current epoch of cosmic acceleration” (Riess et al. 2004).
The deceleration parameter (q0 = ΩM/2) gives an idea how the expansion of the Universe decelerates.
Surprisingly, when the expansion rate data was analysed in terms of mass density (ΩM), ΩM was found to be –0.36. Since there is no such thing as negative mass, therefore, getting a negative value for the mass density made no sense, unless the Universe was accelerating (Riess 2012).
Since q0 = ΩM/2, therefore, a negative value for the mass density (ΩM) clearly implied a negative value for the deceleration parameter (q0) (a positive value for the deceleration parameter (q0 > 0) implies deceleration, whereas a negative value for the deceleration parameter (q0 < 0) implies acceleration).
On introducing cosmological constant “Λ” to the deceleration parameter equation, the equation becomes q0 = (ΩM/2) – ΩΛ (ΩΛ denotes the energy density associated with empty space).
The above equation now helps explain the observed acceleration of the Universe’s expansion under the repulsive influence of an energy component (dark energy). Based on this, the significance of the cosmological constant was calculated, “99.7% to 99.8% confidence no matter what the mass density” (Riess 2012). This strongly confirmed cosmic acceleration.
However, there are problems associated with this.
The apparent transition of Universe’s expansion from deceleration to acceleration cannot be explained without invoking a mysterious and hypothetical energy component (dark energy) of unknown origin having no explanation in fundamental physics.
120-orders-of-magnitude discrepancy involved with it further complicates the problem to an unimaginable extent.
According to Durrer (2011), (as compared to dark matter) “Dark energy, however, is very disturbing. On the one hand, the fact that such an unexpected result has been found by observations shows that present cosmology is truly data driven and not dominated by ideas that can be made to fit sparse observations. Present cosmological data are too good to be brought into agreement with vague ideas. On the other hand, a small cosmological constant is so unexpected and difficult to bring into agreement with our ideas about fundamental physics that people have started to look into other possibilities”.
An experiment conducted by Sabulsky et al. (2019) by using atom interferometry to detect dark energy acting on a single atom placed inside an ultra-high vacuum chamber showed no trace of any mysterious energy.
It is very true that remote supernovae are further away than expected, however, keeping in mind that “people have started to look into other possibilities”, therefore, could there still be another reason that can place remote supernovae further away than expected without acceleration?
Rather than “cosmic deceleration that preceded the current epoch of cosmic acceleration (Riess et al. 2004)”, I strongly suggest “consecutive expansion epochs of the Universe that preceded the current expansion epoch were responsible for placing remote supernovae further away than expected”.
The following observation strongly supports this interpretation – “superluminal remote expansion (expansion >> c)” indicates a slower rate of expansion (deceleration) as compared to “subluminal local expansion (expansion << c)” that indicates a faster rate of expansion (acceleration).
How can superluminal expansion scientifically be justified as deceleration as compared to subluminal expansion? It is completely counterintuitive!
One can explain why remote supernovae are further away than expected without acceleration on the basis of “consecutive expansion epochs of the Universe that preceded the current expansion epoch”.
As expected, the deceleration parameter (q0) also turns out to be negative (q0 < 0) while using such interpretation.
Given below is the abstract from my manuscript along with the link.
The comparison of redshift-distance relationship for high and low-redshift supernovae revealed the surprising transition of Universe’s expansion from deceleration to acceleration. As compared to local supernovae, remote supernovae are further away than expected. The expansion rate obtained for local supernovae is higher with low redshifts as compared to the expansion rate obtained for remote supernovae with high redshifts. Since observed redshifts provide an estimate of recession velocities in order to determine the expansion rate (km/s/Mpc) of the Universe, therefore, it is very disturbing to find that low recession velocities (just 1% of speed of light) indicate a faster rate of expansion (acceleration), whereas high recession velocities (60% of speed of light) indicate a slower rate of expansion (deceleration). In this paper I unravel an undiscovered aspect that perfectly mimics cosmic acceleration. Rather than “cosmic deceleration that preceded the current epoch of cosmic acceleration”, I show in this paper that “consecutive expansion epochs of the Universe that preceded the current expansion epoch were responsible for placing remote supernovae further away than expected”. As a consequence of consecutive expansion, expansion began for remote structures before it did for local structures; remote supernovae are therefore not only further away than expected, but they also happen to yield a slower rate of expansion even with “superluminal expansion velocities”. As a result of consecutive expansion, preceding expansion epochs appear to be decelerating as compared to the expansion epoch that succeeds it. The analysis is based on the redshift-distance relationship plotted for 580 type Ia supernovae from the Supernova Cosmology Project, 7 additional high-redshift type Ia supernovae discovered through the Advanced Camera for Surveys on the Hubble Space Telescope from the Great Observatories Origins Deep Survey Treasury program, and 1 additional very high-redshift type Ia supernova discovered with Wide Field and Planetary Camera 2 on the Hubble Space Telescope. The results obtained by the High-Z Supernova Search Team through observations of type Ia supernovae have also been analysed. The results obtained in this paper have been confirmed by plotting velocity-distance relationship, expansion rate vs. time relationship, expansion factor vs. time relationship, scale factor vs. time relationship, scale factor vs. distance relationship, distance-redshift relationship, and distance modulus vs. redshift relationship, moreover, deceleration parameter (q0) is also found to be negative (q0 < 0).
https://www.researchgate.net/publication/343484700
Answer to PM 2Ring’s comment:
The expansion rate for local structures ranges between 68 km/s/Mpc and 74 km/s/Mpc, whereas for remote structures, the expansion rate ranges between 40 km/s/Mpc and 60 km/s/Mpc.
What we don’t know is the current (present) expansion rate for the remote structures, and, it is simply assumed that the expansion rate derived from the local structures is the present expansion rate for the entire Universe.
According to the Copernican principle, we are not any special or privileged observers, therefore, enforcing or simply assuming that the expansion rate for the entire Universe is the same as the expansion rate for the local Universe also appears to conflict with the Copernican principle since the expansion rate for the local Universe is being prioritized over the entire Universe.
It is not correct to assume that the expansion rate for the entire Universe is the same by prioritizing the local expansion rate over the entire Universe without actually knowing the current (present) expansion rate for the remote structures.
Direct evidence for an accelerating Universe came from observations of type Ia supernovae that showed that remote supernovae are further away than expected as they appeared 10% to 25% dimmer than the local supernovae.
Possibilities included pervasive screen of grey dust between the local and the remote Universe, and the evolution of type Ia supernovae. These possibilities have been addressed and are no longer a concerning factor.
If remote structures began expanding into the Universe before the expansion got initiated for the local structures, then in this case also remote structures would end up being further away than expected. This is exactly what we observe – remote supernovae are indeed further away than expected as compared to the local supernovae.
Now, to prove this that remote structures began expanding into the Universe before the expansion got initiated for the local structures we require a confirmation that would test this possibility.
Direct confirmation for this possibility comes again from analysing those direct observations of type Ia supernovae that made the research team conclude that the Universe is accelerating.
Remote structures are not only further away than expected, but they also yield a slower rate of expansion even with high recession velocities (recession velocities ranging from 30% to 60% of speed of light) as compared to the higher rate of expansion for the local structures even with low recession velocities (recession velocities ranging from 1% to 10% of speed of light).
There can’t be any other reason for such a trend where an object with high recession velocity is not only further away than expected, but is also yielding a slower rate of expansion as compared to the expansion rate obtained for an object with low recession velocity. This is only possible if remote structures began expanding into the Universe before the expansion got initiated for the local structures.
The expansion rate for remote structures ranges between 40 km/s/Mpc and 60 km/s/Mpc – it is not the same for all remote structures, but depends upon their distance and recession velocity, or more precisely when they began expanding into the Universe.
It is not possible that all structures would have expanded at the same time into the Universe, objects with high recession velocity that began expanding before are further away than expected and yield a slower rate of expansion, whereas objects that began expanding comparatively later yield a faster rate of expansion.