Neutron Stars from White Dwarf Mergers: Under 1.4 SM?

AI Thread Summary
The discussion centers on the potential formation of neutron stars from white dwarf mergers, particularly when their combined mass is below the 1.4 solar mass (SM) threshold for a type Ia supernova. Participants express uncertainty about the outcome, with some suggesting that the merger might lead to nuclear fusion rather than direct collapse into a neutron star. Others argue that if the mass remains below the Chandrasekhar limit, the result would likely be a new white dwarf. There is speculation that the merged star could exhibit unique fusion processes before stabilizing. Overall, the conversation highlights the complexities of stellar evolution in low-mass white dwarf mergers.
AdamAutism1998
Messages
28
Reaction score
1
I think this could be a good chance that we see how neutron stars form from White Dwarf mergers. The combined mass of the two are less that than required for a type Ia Supernovae. Won't they merge and collapse into a neutron star? What does everyone else think might happen. I want to be sure if lesser massive degenerate mergers which total under 1.4 SM form neutron stars.
 
AdamAutism1998 said:
I think this could be a good chance that we see how neutron stars form from White Dwarf mergers. The combined mass of the two are less that than required for a type Ia Supernovae. Won't they merge and collapse into a neutron star? What does everyone else think might happen. I want to be sure if lesser massive degenerate mergers which total under 1.4 SM form neutron stars.

Hmmm... I honestly don't know what would happen. I'd guess that the sudden addition of mass would kickstart nuclear fusion and form a new star, not collapse into a neutron star. I'll have to look up more on this.
 
AdamAutism1998 said:
I think this could be a good chance that we see how neutron stars form from White Dwarf mergers. The combined mass of the two are less that than required for a type Ia Supernovae. Won't they merge and collapse into a neutron star?

If combined mass is below Chandrasekhar limit, the end result should be a white dwarf. It's quite likely merged star will have some new ways to achieve fusion, so it may take a while (a few million years?) before it settles into white dwarf state.
 
TL;DR Summary: In 3 years, the Square Kilometre Array (SKA) telescope (or rather, a system of telescopes) should be put into operation. In case of failure to detect alien signals, it will further expand the radius of the so-called silence (or rather, radio silence) of the Universe. Is there any sense in this or is blissful ignorance better? In 3 years, the Square Kilometre Array (SKA) telescope (or rather, a system of telescopes) should be put into operation. In case of failure to detect...
Thread 'Could gamma-ray bursts have an intragalactic origin?'
This is indirectly evidenced by a map of the distribution of gamma-ray bursts in the night sky, made in the form of an elongated globe. And also the weakening of gamma radiation by the disk and the center of the Milky Way, which leads to anisotropy in the possibilities of observing gamma-ray bursts. My line of reasoning is as follows: 1. Gamma radiation should be absorbed to some extent by dust and other components of the interstellar medium. As a result, with an extragalactic origin, fewer...
Both have short pulses of emission and a wide spectral bandwidth, covering a wide variety of frequencies: "Fast Radio Bursts (FRBs) are detected over a wide range of radio frequencies, including frequencies around 1400 MHz, but have also been detected at lower frequencies, particularly in the 400–800 MHz range. Russian astronomers recently detected a powerful burst at 111 MHz, expanding our understanding of the FRB range. Frequency Ranges: 1400 MHz: Many of the known FRBs have been detected...
Back
Top