Evidence for interacting dark energy from BOSS

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SUMMARY

The discussion centers on the paper "Evidence for interacting dark energy from BOSS," which challenges the conventional understanding that dark matter and dark energy do not interact. The paper suggests that both components, typically treated as independent in the ΛCDM model, may have interactions that could explain certain cosmological phenomena. However, concerns are raised regarding the reliability of the data, particularly due to the BOSS survey's limitations in observing quasars at high redshifts and the paper's reliance on a 2-sigma result, which is often deemed inconclusive.

PREREQUISITES
  • Understanding of the Λ-cold-dark-matter (ΛCDM) model
  • Familiarity with cosmological concepts such as dark matter and dark energy
  • Knowledge of statistical significance in scientific research, particularly the implications of 2-sigma results
  • Experience with observational cosmology and the BOSS survey methodology
NEXT STEPS
  • Research the implications of dark energy interactions on cosmological models
  • Examine follow-up studies that cite the paper "Evidence for interacting dark energy from BOSS"
  • Learn about the limitations of the BOSS survey in high-redshift quasar observations
  • Investigate alternative models of dark energy that address current theoretical challenges
USEFUL FOR

Astronomers, cosmologists, and astrophysicists interested in the dynamics of dark matter and dark energy, as well as researchers analyzing observational data from the BOSS survey.

wolram
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https://arxiv.org/pdf/1412.2777.pdf

I have always thought that Dark matter and Dark energy do not interact, but this paper says otherwise.
Just because both are called Dark as a' place name for them' people think they must be akin to one another,
I have always been told this is incorrect

One of the biggest challenges in cosmology and astrophysics nowadays is to understand the nature of the two most abundant components of the Universe: dark energy and dark matter. These are usually described as two independent components where dark matter is responsible for most of the nonrelativistic matter in the Universe and where dark energy is responsible for the late time acceleration of our Universe, which is described by a cosmological constant in the Λ-cold-dark-matter (ΛCDM) model. This standard model is widely used to describe the cosmological evolution of the Universe [1], and it fits very well the current observational data. However, this model has some theoretical and observational challenges (see, e.g., Ref. [2]) that open the way for alternative models of dark energy.
 
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I'll be curious to see follow-ups, but this sentence in the introduction immediately makes me feel extra suspicious:
We point out that BOSS is not optimized to observe quasars at such high redshifts.
This makes it sound like they're including data that is at the limits of detection of the survey. That's always risky. It's also just barely above a 2-sigma result. Most of those turn out to be wrong.

Will have to see what follow-ups have to say. Did you manage to examine any papers that cite this one? It's been a couple of years, so there's at least a chance that this paper has received some substantial replies in the mean time. Looks like it picked up 7 citations, which honestly isn't great. I haven't looked into any of those citations, though.
 
Thanks for the reply kimbyd, I will certainly look up these papers, but as you say 2 sigma is very vague.
 

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