Status of Cosmic Strings and Stringy Inflation

In summary, cosmic strings are considered an alternative to inflation for the formation of structure in the early universe, but have been largely ruled out by WMAP data. They may still exist, but would have a minimal contribution to structure formation. The existence of cosmic strings is not necessarily related to string theory or string cosmology.
  • #1
twistor
74
8
Which is the status of cosmic strings? Could they be related to inflation? Which are the most promising scenarios in which inflation arises/could arise in some way from a string cosmology?
What do you think of the following papers?
http://arxiv.org/abs/hep-th/0507205
http://arxiv.org/abs/hep-ph/9812483?
 
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  • #2
This seems like a homework assignment or project so before we can help why not elaborate more on what you think? this would allow others to comment better on your understanding of the topic.
 
  • #3
Cosmic strings are generally considered as an alternative to inflation when it comes to the formation of structure in the early universe. They were competitors for a while until WMAP showed that the density perturbations were dominantly adiabatic which is a hallmark prediction of inflation, not cosmic strings. It is still possible that cosmic strings formed in the early universe and they they contributed to structure formation, but they would contribute a very small amount.

Note that cosmic strings are not necessarily related to string theory or string cosmology -- different kind of string.
 
  • #4
So they could be out there (cosmic strings), but would have little contribution to structure formation. Is that right?
 
  • #5
twistor said:
So they could be out there (cosmic strings), but would have little contribution to structure formation. Is that right?
Yes. I don't recall the upper limits, though.
 

Related to Status of Cosmic Strings and Stringy Inflation

1. What is the current status of cosmic strings and stringy inflation?

Cosmic strings are hypothetical one-dimensional objects proposed by string theory as a possible explanation for the formation of large-scale structures in the universe. Stringy inflation is a type of cosmic inflation driven by scalar fields in string theory. Currently, there is no direct evidence for the existence of cosmic strings or stringy inflation, but they are still actively studied and debated among scientists.

2. How are cosmic strings and stringy inflation related to each other?

Cosmic strings are considered a potential outcome of stringy inflation, as they could have been formed during the rapid expansion of the universe in the early stages of the Big Bang. Stringy inflation also provides a theoretical framework for understanding the properties and behavior of cosmic strings.

3. What are some proposed methods for detecting cosmic strings?

One proposed method is to look for gravitational lensing effects caused by the presence of cosmic strings. Another method is to search for distortions in the cosmic microwave background radiation, which could be a result of cosmic strings interacting with the radiation. Additionally, some scientists are investigating the possibility of detecting gravitational waves produced by cosmic string collisions.

4. Are there any observational hints or evidence for cosmic strings?

There have been some possible observational hints, such as the alignment of quasars and galaxies along the same direction, which could be caused by the gravitational effects of cosmic strings. However, these hints are still subject to debate and further investigation is needed to confirm the existence of cosmic strings.

5. How does the study of cosmic strings and stringy inflation contribute to our understanding of the universe?

The study of cosmic strings and stringy inflation is important because it provides a deeper understanding of the fundamental laws and forces that govern the universe. It also offers potential explanations for some of the biggest mysteries in cosmology, such as the origin of large-scale structures and the nature of dark matter and dark energy. Additionally, it allows for the development of new theories and models to be tested and refined through observations and experiments.

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