It is generally accepted that only simple Hydrogen (one proton) appeared from the big bang, with a small quantity of heaver isotopes of hydrogen such as deuterium etc which also have the one proton that defines hydrogen but more neutrons are possible including not only deuterium but the unstable isotope of hydrogen called tritium.
A smaller amount of Helium and heavier isotopes were also believed to have formed right up to but not heavier than beryllium. A few BBN theories have been around since the 1940s and they are all an attempt to explain why these elements (Hydrogen in its variations and Helium etc) appeared after the big bang.
Big bang nucleosynthesis
Stellar nucleosynthesis refers to the process by which elements are formed within stars through nuclear fusion during their lifecycles, primarily converting hydrogen into helium and heavier elements in later stages. In contrast, big bang nucleosynthesis occurred in the first few minutes after the Big Bang, resulting in the formation of the lightest elements, primarily hydrogen, helium, and trace amounts of lithium and beryllium. While stellar nucleosynthesis builds upon the elements formed during the big bang, it occurs under different conditions and leads to the creation of heavier elements over billions of years.
The first nucleosynthesis is thought to have occurred shortly after the Big Bang, where simple elements like hydrogen and helium were formed. This initial phase of nucleosynthesis laid the foundation for the creation of more complex elements in stars and supernovae over time.
The process is called nucleosynthesis. After the Big Bang, the nucleosynthesis process involved the fusion of hydrogen and helium nuclei to form elements like lithium, beryllium, and some trace amounts of heavier elements.
Three minutes after the Big Bang, the universe had cooled down enough for protons and neutrons to begin combining to form the first atomic nuclei, a process known as nucleosynthesis. This marks the beginning of the era of light nuclei formation in the early universe.
Big bang nucleosynthesis
Stellar nucleosynthesis refers to the process by which elements are formed within stars through nuclear fusion during their lifecycles, primarily converting hydrogen into helium and heavier elements in later stages. In contrast, big bang nucleosynthesis occurred in the first few minutes after the Big Bang, resulting in the formation of the lightest elements, primarily hydrogen, helium, and trace amounts of lithium and beryllium. While stellar nucleosynthesis builds upon the elements formed during the big bang, it occurs under different conditions and leads to the creation of heavier elements over billions of years.
The first nucleosynthesis is thought to have occurred shortly after the Big Bang, where simple elements like hydrogen and helium were formed. This initial phase of nucleosynthesis laid the foundation for the creation of more complex elements in stars and supernovae over time.
The process is called nucleosynthesis. After the Big Bang, the nucleosynthesis process involved the fusion of hydrogen and helium nuclei to form elements like lithium, beryllium, and some trace amounts of heavier elements.
Three minutes after the Big Bang, the universe had cooled down enough for protons and neutrons to begin combining to form the first atomic nuclei, a process known as nucleosynthesis. This marks the beginning of the era of light nuclei formation in the early universe.
Big Bang nucleosynthesis produced stable isotopes for:Hydrogen(Deuterium)HeliumLithium
Hydrogen and helium were the two main elements created in abundance during the Big Bang nucleosynthesis. These elements were formed in the first few minutes after the Big Bang, when the universe was hot and dense enough to support nuclear fusion.
In physical cosmology, Big Bang nucleosynthesis refers to the production of nuclei other than those of the lightest isotope of hydrogen during the early phases of the universe.
Hydrogen was formed in the early universe, around 3 minutes after the Big Bang during a phase known as Big Bang nucleosynthesis. At that time, the extremely high temperatures and pressures allowed for the fusion of protons and neutrons to form hydrogen nuclei.
The three stages of the Big Bang are the primordial nucleosynthesis, the recombination era, and the cosmic microwave background radiation era. In primordial nucleosynthesis, the first nuclei formed; during the recombination era, hydrogen atoms formed; and in the cosmic microwave background radiation era, the Universe cooled down enough for light to travel freely.
The first elements were created shortly after the Big Bang, around 13.8 billion years ago. Hydrogen and helium were among the first elements formed in the early universe through nucleosynthesis.
Nucleosynthesis. It refers to the formation of atoms larger than Helium-1. Because of the extreme conditions right after the Big Bang, it is believed that some Deuterium and Helium were formed, perhaps some Lithium too; but no significant amounts of other metals. (In Astronomy, a metal is any element heavier than Helium.)