What is the next step in cosmology

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In summary, advancements in gravitational radiation mapping will not occur until space-based observations are available, leaving us to rely on the still-developing LIGO technology. Other possibilities for improving our understanding of cosmology include detecting primordial B-mode polarization of the CMB, using BH-BH mergers as standard candles, observing the "dark ages" through measuring the 21cm Hydrogen line, and conducting more accurate and larger galaxy surveys to better understand dark energy.
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I think gravitational radiation mapping, but this will not happen until we have space based observations, until then we have to rely on LIGO which is in its infancy.
 
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Some other possibilities:
1. Detection of primordial B-mode polarization of the CMB.
2. Use of BH-BH mergers as standard (or standardizable) candles. I saw a talk a little while ago where they showed that if we could find an optical signal of the event, and in particular measure its redshift, the BH-BH mergers would be vastly more accurate than supernovae as standard candles. I think we'd need three gravity wave observatories to all detect the same event to have a chance of narrowing the location in the sky sufficiently to point telescopes at it before the light fades, if there is any detectable light at all.
3. Observations of the "dark ages" before the stars turned on through measuring the 21cm Hydrogen line (see here).
4. More accurate and larger galaxy surveys to better nail down dark energy. These will be generally slow, incremental improvements, but still important for better understanding of cosmology.
 
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What is the current state of cosmology research?

The current state of cosmology research is constantly evolving as new discoveries and advancements are made. However, some of the key areas of focus in cosmology research include the study of the origins and evolution of the universe, the properties of dark matter and dark energy, and the search for evidence of other universes or dimensions.

What is the next step in understanding the Big Bang theory?

The next step in understanding the Big Bang theory is to gather more precise measurements of the cosmic microwave background radiation, which is the remnant heat from the early universe. This will help us to better understand the conditions of the universe in its earliest stages and potentially provide clues about the existence of inflation, a rapid expansion that occurred in the early universe.

How will advancements in technology impact cosmology research?

Advancements in technology, such as powerful telescopes and detectors, will greatly impact cosmology research by allowing us to observe and measure the universe in more detail than ever before. This will help us to better understand the properties of dark matter and dark energy, as well as potentially discover new information about the origins and evolution of the universe.

What role does dark matter and dark energy play in cosmology?

Dark matter and dark energy are two of the biggest mysteries in cosmology. Dark matter is believed to make up about 27% of the universe and plays a crucial role in the formation and structure of galaxies. Dark energy, on the other hand, is thought to make up about 68% of the universe and is responsible for the accelerated expansion of the universe.

How are scientists testing theories about the multiverse?

Currently, scientists are using a variety of methods to test theories about the multiverse, which is the idea that our universe is just one of many parallel universes. These methods include studying the cosmic microwave background radiation, looking for gravitational waves, and searching for evidence of a collision between our universe and another. However, the concept of the multiverse is still highly speculative and remains a topic of ongoing debate among scientists.

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