Notes 2: Difference between revisions
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Atomic nuclei sizes are on the scale of <math>10^{-14} </math> meters and form the (relatively) small centers of atoms while carrying most of the mass. The basic constituents of atomic nuclei are protons and neutrons. Protons and neutrons are comprised of three quarks each, fundamental particles on a size scale of <math> 10^{-19} m </math>. The relevant interactions on this size/mass scale are the electro-weak and strong forces. The quarks in a nucleon are | Atomic nuclei sizes are on the scale of <math>10^{-14} </math> meters and form the (relatively) small centers of atoms while carrying most of the mass. The basic constituents of atomic nuclei are protons and neutrons. Protons and neutrons are comprised of three quarks each, fundamental particles on a size scale of <math> 10^{-19} m </math>. The relevant interactions on this size/mass scale are the electro-weak and strong forces. The quarks in a nucleon are | ||
Since Becquerel and Rutherford, much has been learned about nuclear physics. We now know that the atom is much more complex than Bohr's planetary like model could hope to explain. For instance, matter is not the lone constituent of the universe. There is also antimatter (save dark energy and matter for another day) with identical spin and mass but opposite charge. It seems for each massive particle, there is an antimatter equivalent denoted with a bar over its symbol. | Since Becquerel and Rutherford, much has been learned about nuclear physics. We now know that the atom is much more complex than | ||
Bohr's planetary like model could hope to explain. For instance, matter is not the lone constituent of the universe. There is also | |||
antimatter (save dark energy and matter for another day) with identical spin and mass but opposite charge. It seems for each massive | |||
particle, there is an antimatter equivalent denoted with a bar over its symbol. | |||
The composition of the nucleus is on the most basic level comprised of protons (Z) and neutrons (N) | The composition of the nucleus is on the most basic level comprised of protons (Z) and neutrons (N) | ||
Revision as of 01:17, 24 January 2011
Nuclear Astrophysics is a combination of nuclear physics and astrophysics. Nuclear physics is the study of atomic nuclei, their composition and their interactions, while astrophysics aims at studying galactic objects such as stars and galaxies. Nuclear astrophysics delves into the questions of where and when the elements were created and how nuclear reactions drive cosmic events.
The Nucleus
Atomic nuclei sizes are on the scale of Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle 10^{-14} } meters and form the (relatively) small centers of atoms while carrying most of the mass. The basic constituents of atomic nuclei are protons and neutrons. Protons and neutrons are comprised of three quarks each, fundamental particles on a size scale of Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle 10^{-19} m } . The relevant interactions on this size/mass scale are the electro-weak and strong forces. The quarks in a nucleon are
Since Becquerel and Rutherford, much has been learned about nuclear physics. We now know that the atom is much more complex than
Bohr's planetary like model could hope to explain. For instance, matter is not the lone constituent of the universe. There is also antimatter (save dark energy and matter for another day) with identical spin and mass but opposite charge. It seems for each massive particle, there is an antimatter equivalent denoted with a bar over its symbol.
The composition of the nucleus is on the most basic level comprised of protons (Z) and neutrons (N)
Definitions for Abundance
The particle abundance of isotope Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle i } is defined as
- Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle X_{i} = \frac{n_i}{\sum_j n_j} \, }
where Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle n_i } is the the number density of particle Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle i } , and the sum is taken over all isotopes present. It is also useful to define a relative particle abundance, which is set logarithmically and normalized to the abundance of hydrogen:
- Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \epsilon_i = \log_{10} X_i + 12 \ . }
The mass fraction is the fraction of total mass in the sample constituted by species Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle i } :
- Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle X_i = \frac{m_i}{m_{tot}} = \frac{m_i n_i}{\rho} \approx \frac{A_i n_i}{\rho N_A} } ( Note that Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle m_i \approx A_i m_u \ } and Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle m_u = \frac{m_{12C}}{12} = \frac{1}{N_A} } )
Denoting Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle Y_i\,} the mass per baryon, as
- Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle Y_i \equiv \frac{X_i}{A_i} , }
allows us to define the particle's number density by the density of the sample and this baryon fraction,
- Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle n_i = Y_i \rho N_A \ . }
Another useful quantity is the average mass number, or mean molecular weight, defined by
- Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \mu_i = \frac{\sum_i{A_i Y_i}}{\sum_i{Y_i}} = \frac{\sum_i{N_i}}{\sum_iY_i} = \frac{1}{\sum_i{Y_i}}}
The electron abundance
- Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle Y_e = \sum_i Z_i Y_i \ } , which can also be written as Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle Y_e = \frac{\sum_i{Z_i Y_i}}{\sum_i{A_i Y_i}} ,}
is the ratio of protons to nucleons in the sample, and similarly to nuclei, the electron number density is found by
- Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle n_e = Y_e \rho N_A \ . }