Readings

Tamsioji energija: paslaptinga jėga, skatinanti kosminę plėtrą

Dark energy: a mysterious force driving cosmic ...

Dark energy is a mysterious component of the Universe causing its accelerated expansion. Although it constitutes the majority of the Universe's total energy density, its exact nature remains one of...

Dark energy: a mysterious force driving cosmic ...

Dark energy is a mysterious component of the Universe causing its accelerated expansion. Although it constitutes the majority of the Universe's total energy density, its exact nature remains one of...

Tamsioji materija: kaip atskleisti Visatos nematomąją masę

Dark matter: how to reveal the invisible mass o...

Dark matter – one of the greatest mysteries of modern astrophysics and cosmology. Although it makes up the majority of the Universe's matter, its nature remains unclear. Dark matter neither...

Dark matter: how to reveal the invisible mass o...

Dark matter – one of the greatest mysteries of modern astrophysics and cosmology. Although it makes up the majority of the Universe's matter, its nature remains unclear. Dark matter neither...

Kosminė foninė mikrobangė spinduliuotė (KFMS)

Cosmic background microwave radiation (CBMR)

The remaining radiation from the time when the Universe became transparent about 380,000 years after the Big Bang The Cosmic Microwave Background (CMB) is often described as the oldest light...

Cosmic background microwave radiation (CBMR)

The remaining radiation from the time when the Universe became transparent about 380,000 years after the Big Bang The Cosmic Microwave Background (CMB) is often described as the oldest light...

Aušimas ir pamatinių dalelių formavimasis

Cooling and formation of fundamental particles

Cooling and formation of fundamental particles As the Universe cooled from extremely high temperatures, quarks combined into protons and neutrons One of the most important early Universe epochs was the...

Cooling and formation of fundamental particles

Cooling and formation of fundamental particles As the Universe cooled from extremely high temperatures, quarks combined into protons and neutrons One of the most important early Universe epochs was the...

Medžiaga prieš antimateriją

Material against antimatter

Matter vs. Antimatter: the imbalance that allowed matter to dominate One of the deepest mysteries of modern physics and cosmology is why our The Universe consists almost entirely of matter,...

Material against antimatter

Matter vs. Antimatter: the imbalance that allowed matter to dominate One of the deepest mysteries of modern physics and cosmology is why our The Universe consists almost entirely of matter,...

Didžiojo sprogimo nukleosintezė (BBN)

Big Bang nucleosynthesis (BBN)

Big Bang nucleosynthesis (BBN) marks a brief period—roughly from 1 second to 20 minutes after the Big Bang—when the Universe was hot and dense enough for nuclear fusion to form...

Big Bang nucleosynthesis (BBN)

Big Bang nucleosynthesis (BBN) marks a brief period—roughly from 1 second to 20 minutes after the Big Bang—when the Universe was hot and dense enough for nuclear fusion to form...