Time and Universe: Shedding Light on Dark Energy & Dark Matter

In summary, the conversation discusses a paper on the nature of cosmological time, which suggests that the flow of time is dependent on the dynamical state of the Universe rather than being constant. This alternative hypothesis is based on the relationship between time and entropy, and the paper presents a cosmological model that explains Type Ia Supernovae data without the need for dark matter or dark energy. However, upon review, it is determined that the paper is not peer reviewed and may not be a reliable source. As a result, the conversation is closed.
  • #1
wolram
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I found this article interesting it does away with dark energy and dark matter. two of the things i hate in cosmology.

On the nature of cosmological time
Pierre Magain, Clémentine Hauret
Comments: 5 pages, 4 figures, submitted to MNRAS
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO); General Relativity and Quantum Cosmology (gr-qc)
Time is a parameter playing a central role in our most fundamental modeling of natural laws. Relativity theory shows that the comparison of times measured by different clocks depends on their relative motions and on the strength of the gravitational field in which they are embedded. In standard cosmology, the time parameter is the one measured by fundamental clocks, i.e. clocks at rest with respect to the expanding space. This proper time is assumed to flow at a constant rate throughout the whole history of the Universe. We make the alternative hypothesis that the rate at which cosmological time flows depends on the dynamical state of the Universe. In thermodynamics, the arrow of time is strongly related to the second law, which states that the entropy of an isolated system will always increase with time or, at best, stay constant. Hence, we assume that time measured by fundamental clocks is proportional to the entropy of the region of the Universe that is causally connected to them. Under that simple assumption, we build a cosmological model that explains the Type Ia Supernovae data (the best cosmological standard candles) without the need for exotic dark matter nor dark energy.
 
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  • #2
On review, it does not appear that this paper is peer reviewed, and it does not appear to be a reputable source. Thread closed.
 
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1. What is dark energy and dark matter?

Dark energy and dark matter are two mysterious and elusive components of the universe. Dark energy is an unknown force that is believed to be responsible for the accelerating expansion of the universe. Dark matter is a type of matter that does not interact with light and cannot be seen, but it makes up about 27% of the universe's total mass.

2. How are dark energy and dark matter related to time?

Dark energy and dark matter play a crucial role in the evolution of the universe over time. Dark energy's presence is believed to be the reason for the accelerating expansion of the universe, while dark matter's gravity helps to hold galaxies and large-scale structures together over time.

3. How do scientists study dark energy and dark matter?

Scientists use a variety of methods to study dark energy and dark matter, including observations of the cosmic microwave background radiation, galaxy clusters, and the large-scale structure of the universe. They also conduct experiments using particle accelerators, such as the Large Hadron Collider, to try and detect dark matter particles.

4. What is the current understanding of dark energy and dark matter?

While dark energy and dark matter remain mostly mysterious, scientists have made some progress in understanding their properties. The most widely accepted theory is that dark energy is a form of energy that fills the entire universe and has a negative pressure that is causing the expansion of the universe to accelerate. Dark matter is believed to be made up of particles that interact only through gravity and has not yet been directly detected.

5. How do dark energy and dark matter impact the future of the universe?

The presence of dark energy and dark matter will continue to shape the future of the universe. Dark energy's influence is expected to cause the universe to expand at an increasing rate, eventually leading to the "Big Rip," where all matter in the universe will be torn apart. Dark matter's gravitational pull will continue to play a role in the formation and evolution of galaxies and large-scale structures over time.

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