Nucleosynthesis and light curve of Supernovae Ia

In summary, type Ia supernova is the complete disruption of a white dwarf after passing through the deflagration and detonation phases. Before these phases, carbon, oxygen, and silicon undergo hydrostatic nuclear reactions as density and temperature increase in the white dwarf. The specific nuclear reactions occurring at the deflagration and detonation phase are complex and simulated through a reaction network. The explosion process produces silicon, iron, and cobalt in varying ratios, and the Si II line in the light curve is intense due to the large amount of silicon produced from the fusion of C+O. The products of silicon burning are not fully formed before the explosion, and the Si II line is prominent in type Ia supernovas because it is concentrated
  • #1
elouisa
1
0
Hi all,

I am trying to understand the connection between the specific nucleosynthesis that occurs in each step of the explosion mechanism of type Ia supernova (SN Ia).

Let´s see if I got it right, type Ia SN is the complete disruption of a white dwarf(WD) once it passes through the deflagration and detonation phases. Before those phases, as density and temperature increases in the WD, carbon, oxygen and silicon burns. These would be hydrostatic nuclear reactions, right?. Now, my questions are:
Which are the specific nuclear reactions occurring at the degflagration and detonation phase?
Which are the specific so called explosive nucleosynthesis happening in this type of supernova?
Do all the products of the silicon burning are ¨cooked¨ before the explosion?
Which are the specific elements produced during the deflagration and detonation phases?

And about the light curve, why the Si II line is so intense?


Thank you very much!
 
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  • #2
elouisa said:
Which are the specific nuclear reactions occurring at the degflagration and detonation phase?

This is a *VERY* complicated question. The way that people simulate everything is by having a reaction network which calculates the speed at which one isotope gets converted to another isotope a given temperature and pressure. Typically these calculations simulate several hundred different nuclear reactions.

http://arxiv.org/abs/astro-ph/0505417

Do all the products of the silicon burning are ¨cooked¨ before the explosion?

No. The explosion cooks them. There's no new silicon in a supernova Ia before the explosion. The silicon gets produced during the explosion.

Which are the specific elements produced during the deflagration and detonation phases?

Rather complicated question. What happens is that because detonation is a more violent process, you end up with heavier isotopes (iron and cobalt) than with deflagration. It's not so much specific elements as ratios between different isotopes. Also, you see fast moving iron and cobalt in Ia's which says that there is some sort of detonation, but if the whole explosion were a detonation you'd end up with too much heavy element.

And about the light curve, why the Si II line is so intense?

Because large amounts of C+O fuse in the explosion to form silicon. This contrasts with Ib's and Ic's which are basically type II supernova whose hydrogen envelope has been stripped, and in which there isn't the large amount of silicon because it's already been burned to iron.
 
  • #3
twofish-quant said:
Because large amounts of C+O fuse in the explosion to form silicon. This contrasts with Ib's and Ic's which are basically type II supernova whose hydrogen envelope has been stripped, and in which there isn't the large amount of silicon because it's already been burned to iron.

To add, the least dense material in the WD at the surface burns to Si (denser burning leads to heavier nuclei, mostly Ni56). So not only is Si the product of the burning, but its concentrated at the surface, and so is a component of the photosphere right from the beginning.
 

1. What is nucleosynthesis and how does it relate to Supernovae Ia?

Nucleosynthesis is the process by which elements are created in the universe. It is responsible for the formation of all elements heavier than hydrogen and helium. Supernovae Ia are a type of supernova explosion that occurs in binary star systems, where one star is a white dwarf. During these explosions, nucleosynthesis occurs, creating new elements and spreading them throughout the universe.

2. How do scientists study the light curve of Supernovae Ia?

Scientists study the light curve of Supernovae Ia by observing the changes in brightness over time. They use telescopes and other instruments to collect data on the supernova's luminosity and how it changes over weeks and months. This information can provide valuable insights into the nature of the explosion and the elements involved.

3. What is the significance of studying the light curve of Supernovae Ia?

Studying the light curve of Supernovae Ia allows scientists to gain a better understanding of the physics behind these explosive events. It also helps them to determine the distance of the supernova from Earth, which can be used to measure the expansion rate of the universe and investigate the effects of dark energy.

4. What elements are created during nucleosynthesis in Supernovae Ia?

Nucleosynthesis in Supernovae Ia results in the creation of many elements, including iron, nickel, silicon, and sulfur. These elements are essential building blocks for planets, stars, and life as we know it. The exact elements created can vary depending on the conditions of the explosion.

5. Can the light curve of Supernovae Ia be used to determine the age of the universe?

Yes, the light curve of Supernovae Ia can be used to determine the age of the universe. By measuring the distance of a supernova and its redshift, scientists can calculate the rate of expansion of the universe. This information, combined with other data, can be used to estimate the age of the universe.

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