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1 030 (0,139s) •

Project

New Precision Tests of the Dark Sector (GA24-10780S)

dark matter (25% of the energy budget), but also dark energy (DE, 70% of the energy budget). While these dark components have been extensively studied and constrained......

Particles and field physics

  • 2024 - 2026
    • •
  • 10 601 tis. Kč
    • •
  • 8 232 tis. Kč
    • •
  • GA ČR
Project

Cosmology, Gravity and the Dark Sector of the Universe (EF15_003/0000437)

The CoGraDS project is focused on research on key cosmology topics, namely the nature of dark matter and dark energy and the validity of Einstein's general theory of relativity in the context of current and planned European and Amer...

JV - Kosmické technologie

  • 2016 - 2023
    • •
  • 160 588 tis. Kč
    • •
  • 157 366 tis. Kč
    • •
  • MŠMT
Project

DArk matter, NeUtrinos and BEyond (DAvBE) (8X25051)

Despite the theoretical appeal of portal particles as a bridge between visible and dark sectors, developing a comprehensive theoretical framework remains challenging. The physics of such portals spans an enormous range of energy sca...

Particles and field physics

  • 2025 - 2027
    • •
  • 227 tis. Kč
    • •
  • 227 tis. Kč
    • •
  • MŠMT
Project

Strong Gravity as a Microscope for the Dark Universe (GA20-28525S)

Observations firmly established that the 70% of our universe consists of dark energy, while a further 25 % of dark matter. The nature and origin of both dark that on cosmological scales, dark matter behaves like du...

Particles and field physics

  • 2020 - 2023
    • •
  • 13 001 tis. Kč
    • •
  • 12 335 tis. Kč
    • •
  • GA ČR
Project

New avenues in the hunt for dark energy (GM21-16583M)

This is an interdisciplinary programme bridging cosmology, astrophysics and particle physics towards explaining dark energy in the Universe. The resolution of dark for fifth forces in Nature. Within generic theories for dark

Astronomy (including astrophysics,space science)

  • 2021 - 2025
    • •
  • 17 183 tis. Kč
    • •
  • 17 183 tis. Kč
    • •
  • GA ČR
Project

Spin 2 WISPers from the laboratory to the cosmos (LUC23115)

There exists multiple evidence for the fact that the Universe comprises 25% dark matter, slow-moving particles which interact weakly with visible matter experimental effort and expectations, dark matter has not been detected on Eart...

Particles and field physics

  • 2023 - 2025
    • •
  • 6 074 tis. Kč
    • •
  • 6 074 tis. Kč
    • •
  • MŠMT
Project

Functional species pools shedding light on the dark diversity and its functions (GAP505/12/1296)

from an ecosystem, but belonging to its species pool, constitutes the dark diversity of a site. Properly estimating the dark diversity of a site is essential on dark diversity, we aim at (i) comparing different techniques ...

EF - Botanika

  • 2012 - 2016
    • •
  • 11 682 tis. Kč
    • •
  • 11 682 tis. Kč
    • •
  • GA ČR
Project

Implications of non-standard particle and gravitational models for cosmology. (GJ20-16531Y)

, which can account for Dark Matter or explain baryon asymmetry of the Universe introducing Dark Energy. We will examine viability of these models throughout......

Particles and field physics

  • 2020 - 2022
    • •
  • 10 945 tis. Kč
    • •
  • 10 945 tis. Kč
    • •
  • GA ČR
Project

The origin of dark neutral gas structures around galaxies (GA19-18647S)

We will investigate the formation and evolution of optically dark neutral gas structures detected in the Arecibo Galaxy Environment Survey. Among the most intriguing, implying a high dark matter content. If so such objects would be ...

Astronomy (including astrophysics,space science)

  • 2019 - 2022
    • •
  • 5 217 tis. Kč
    • •
  • 5 154 tis. Kč
    • •
  • GA ČR
Project

Privatization of Security Role of Private Sector Actors in Countering Contemporary Security Threats (GAP408/11/0395)

, cybersecurity etc. The project will also explore the dark side of security privatization...

AD - Politologie a politické vědy

  • 2011 - 2015
    • •
  • 3 396 tis. Kč
    • •
  • 3 296 tis. Kč
    • •
  • GA ČR
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