cosmic:start
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cosmic:start [2022/07/19 11:51] – [Description] kristi.engel | cosmic:start [2022/11/02 17:10] (current) – Added arxiv links kadrlica | ||
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====== COSMIC FRONTIER ====== | ====== COSMIC FRONTIER ====== | ||
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===== Conveners ===== | ===== Conveners ===== | ||
^Name ^Institution ^Email | | ^Name ^Institution ^Email | | ||
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- | * [[https://urldefense.proofpoint.com/v2/url?u=https-3A__www.overleaf.com_read_fjvszqjyrnpy& | + | * [[https://arxiv.org/abs/2209.07426 | CF1 Topical Group Report]] |
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* {{ : | * {{ : | ||
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This group covers dark matter in the regime where it appears in experiments as individual quanta, rather than coherently via wave phenomena. Techniques to search for such particles include directly through its interaction with detector materials, indirectly from products of its annihilation, | This group covers dark matter in the regime where it appears in experiments as individual quanta, rather than coherently via wave phenomena. Techniques to search for such particles include directly through its interaction with detector materials, indirectly from products of its annihilation, | ||
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- | * {{ :cosmic: | + | * [[https://arxiv.org/ |
* [[https:// | * [[https:// | ||
* {{ : | * {{ : | ||
* [[https:// | * [[https:// | ||
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This group covers low mass bosonic dark matter in the regime where it appears in experiments coherently via wave phenomena rather than as individual quanta. Examples include the QCD axion and more general axions, dark photons, and scalar dark matter. Current experimental techniques include broadband and resonant searches via cavities, circuit oscillators, | This group covers low mass bosonic dark matter in the regime where it appears in experiments coherently via wave phenomena rather than as individual quanta. Examples include the QCD axion and more general axions, dark photons, and scalar dark matter. Current experimental techniques include broadband and resonant searches via cavities, circuit oscillators, | ||
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- | * {{ :cosmic: | + | * [[https://arxiv.org/ |
* [[https:// | * [[https:// | ||
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This group covers properties of dark matter that can be uniquely probed by cosmological and astrophysical observations. Techniques include measurements of the cosmological distribution of dark matter, as well as studies of astrophysical objects in extreme environments. Examples of dark matter models probed through these techniques are warm dark matter, self-interacting dark matter, ultra-light axions, and primordial black holes. | This group covers properties of dark matter that can be uniquely probed by cosmological and astrophysical observations. Techniques include measurements of the cosmological distribution of dark matter, as well as studies of astrophysical objects in extreme environments. Examples of dark matter models probed through these techniques are warm dark matter, self-interacting dark matter, ultra-light axions, and primordial black holes. | ||
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- | * {{ :cosmic: | + | * [[https://arxiv.org/ |
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* {{ : | * {{ : | ||
* [[https:// | * [[https:// | ||
- | * {{ :cosmic:cssv1_DEcomp.pdf| CSS Parallel | + | * {{ :cosmic:repdiscv1_cf4.pdf | CSS Report Discussion |
This group covers cosmic probes of cosmology in the Modern Universe, when galaxies are fully formed. These probes include galaxy clusters, galaxy clustering, redshift space distortions, | This group covers cosmic probes of cosmology in the Modern Universe, when galaxies are fully formed. These probes include galaxy clusters, galaxy clustering, redshift space distortions, | ||
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- | * [[https://urldefense.proofpoint.com/v2/url? | + | * {{ : |
+ | * [[https://docs.google.com/spreadsheets/d/ | ||
* {{ : | * {{ : | ||
- | * {{ :cosmic:cssv1_DEcomp.pdf| CSS Parallel | + | * {{ :cosmic:repdiscv1_cf5.pdf | CSS Report Discussion |
This group covers cosmic probes of cosmology in the early Universe from Inflation Era through the Cosmic Dawn. Subtopics include: growth of structure probes (e.g. 21cm power spectrum in the dark ages), probes of expansion history (e.g. BAO with black hole mergers, CMB), primordial non-gaussianity and inflation. High-z gravitational wave observatories, | This group covers cosmic probes of cosmology in the early Universe from Inflation Era through the Cosmic Dawn. Subtopics include: growth of structure probes (e.g. 21cm power spectrum in the dark ages), probes of expansion history (e.g. BAO with black hole mergers, CMB), primordial non-gaussianity and inflation. High-z gravitational wave observatories, | ||
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- | * {{ :cosmic: | + | * [[https://arxiv.org/ |
- | * [[https://urldefense.proofpoint.com/v2/url? | + | * [[https://docs.google.com/document/d/ |
* {{ : | * {{ : | ||
- | * {{ :cosmic:cssv1_DEcomp.pdf| CSS Parallel | + | * {{ :cosmic:repdiscv1_cf6.pdf | CSS Report Discussion |
This group covers the connections between probes across multiple axes including combined probes across the early/late time regimes, and plans for future observatories/ | This group covers the connections between probes across multiple axes including combined probes across the early/late time regimes, and plans for future observatories/ | ||
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- | * {{ :cosmic:cssv1_cf7.pdf| CSS Parallel Slides CF7 (Jul. 19)}} | + | * {{ :cosmic:cssv2_cf7.pdf| CSS Parallel Slides CF7 (Jul. 19)}} |
+ | * [[https:// | ||
* [[https:// | * [[https:// | ||
- | * {{ :cosmic:cssv1_DEcomp.pdf| CSS Parallel | + | * {{ :cosmic:repdiscv3_cf7.pdf | CSS Report Discussion |
CF7 covers cosmic probes of fundamental physics topics beyond Dark Matter and Dark Energy using gravitational waves, cosmic rays, gamma rays, and neutrinos, as well as their combined studies to facilitate the multi-messenger science. This includes measurements of neutrino properties from cosmology (overlap with NF 5), tests of general relativity, emergent spacetime (overlap with CF2, 3, 5), black hole information with gravitational waves, the tension between local distance ladder measurements and cosmic microwave background estimates of the Hubble constant, equation of state of dense nuclear matter and hadron-quark gluon phase transitions, | CF7 covers cosmic probes of fundamental physics topics beyond Dark Matter and Dark Energy using gravitational waves, cosmic rays, gamma rays, and neutrinos, as well as their combined studies to facilitate the multi-messenger science. This includes measurements of neutrino properties from cosmology (overlap with NF 5), tests of general relativity, emergent spacetime (overlap with CF2, 3, 5), black hole information with gravitational waves, the tension between local distance ladder measurements and cosmic microwave background estimates of the Hubble constant, equation of state of dense nuclear matter and hadron-quark gluon phase transitions, |
cosmic/start.1658249508.txt.gz · Last modified: 2022/07/19 11:51 by kristi.engel