Searching for Dark Matter in 3.5 Kev Line Mystery

  • Thread starter Chronos
  • Start date
  • Tags
    Line
In summary, the 3.5 Kev x-ray emission line, first reported in 2014, is still being discussed in the literature. A recent paper contradicts earlier findings, but like previous challenges, it appears weak under closer scrutiny. The original team studying the line claims there is more data to come, and the controversy surrounding the line continues.
  • #1
Chronos
Science Advisor
Gold Member
11,440
750
The 3.5 Kev x ray emission line first reported by Bulbul and Boyarsky in early 2014 continues to surface in the literature. This paper;http://arxiv.org/abs/1512.07217, Searching for decaying dark matter in deep XMM-Newton observation of the Draco dwarf spheroidal, conflicts with the findings of Jeltema and Profumo earlier this month claiming no evidence for any such line [re: http://arxiv.org/abs/1512.01239, Deep XMM Observations of Draco rule out a dark matter decay origin for the 3.5 keV line]. Not unlike previous challenges of the 3.5 Kev line as evidence for dark matter decay, this one too appears weak in the face of closer scrutiny. Now, two years following discovery of the 3.5 Kev emission line, it remains a mystery.
 
Space news on Phys.org
  • #2
This is getting perilously close to "splitting hairs on cue-balls" don't you think?
 
  • #3
There was a lot of excitement about this paper and some controversy. The data being published originally belonged to another team who are studying this line. The data became available and these two published it seemingly to try to scoop the other team. However the original team claim that this is not the end and this was the worst data set with solar activity causing problems. I don't put much home in the 3.5 keV line but I think we will have to see what the original team come up with before jumping to conclusions.
 

1. What is dark matter and why is it important to study?

Dark matter is a hypothetical form of matter that does not interact with light, making it invisible to telescopes. It is believed to make up about 85% of the total mass of the universe and plays a crucial role in the formation and evolution of galaxies. Studying dark matter can help us better understand the structure and dynamics of the universe.

2. What is the 3.5 Kev line and why is it important in the search for dark matter?

The 3.5 Kev line is an x-ray emission line that is thought to be produced by the decay of sterile neutrinos, a type of dark matter particle. This line is important because it provides a potential signature of dark matter that can be observed and studied by scientists.

3. How are scientists searching for dark matter using the 3.5 Kev line?

Scientists are using a variety of methods to search for the 3.5 Kev line, including observations with x-ray telescopes and experiments in underground laboratories. These experiments are designed to detect the 3.5 Kev line and measure its properties, which can provide valuable information about the nature of dark matter.

4. What progress has been made in the search for dark matter using the 3.5 Kev line?

While there have been several detections of the 3.5 Kev line in various observations, these detections have not been confirmed and are still under debate. Therefore, there is currently no conclusive evidence for the existence of dark matter particles emitting the 3.5 Kev line. However, ongoing experiments and observations continue to make progress in this search.

5. How does the search for dark matter using the 3.5 Kev line contribute to our understanding of the universe?

Studying the 3.5 Kev line and its potential connection to dark matter can provide insight into the properties and behavior of this elusive substance. It can also help us refine our theories about the nature of dark matter and its role in the universe. Ultimately, the search for dark matter using the 3.5 Kev line is an important step in unraveling the mysteries of our universe and expanding our knowledge of the cosmos.

Similar threads

  • Beyond the Standard Models
Replies
4
Views
1K
  • High Energy, Nuclear, Particle Physics
Replies
15
Views
1K
Replies
20
Views
2K
  • Astronomy and Astrophysics
Replies
1
Views
1K
Replies
93
Views
11K
  • Cosmology
Replies
1
Views
1K
  • Cosmology
Replies
2
Views
1K
Replies
9
Views
2K
Back
Top