Stimulated virtual W+, W- when supernova core-> neutron star?

In summary, under the right conditions, weak interactions allow for the conversion of electrons and protons to neutrons and neutrinos, leading to the formation of a neutron star. This process also produces a large number of virtual W+ and W- bosons in a short time frame. It is uncertain to what extent these virtual bosons stimulate the emission of other virtual W+ and W- bosons in extreme conditions and how the large gravitational well of the core affects these reactions. The degree of coherence between these virtual particles is also uncertain and there is no classical limit for a coherent large amplitude oscillation of the W+ W- field. It is unknown if the massive weak bosons decay quickly or if they have a preference to decay.
  • #1
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Stimulated virtual W+, W- when supernova core--> neutron star?

Weak interactions allow supernova core electrons and protons to convert to neutrons and neutrinos allowing (under the right conditions) the formation of a neutron star? Large numbers virtual W+ and W-bosons are produced in a short time frame (there is a more precise way to state this quantum mechanically)?

To what degree if any do these virtual bosons stimulate emission of other virtual W+ and W-bosons under the most extreme conditions imaginable in a progenitor of the neutron star?

What effect if any does the large gravitational well the core "sits in" have on such reactions?

What is the degree of coherence if any between these virtual particles?

Is there a classical limit of a coherent large amplitude, large extent oscillation of the W+ W- field like there is for the photon field (not worried that such a state is probably not possiible) or do the massive weak bosons "want" to quickly decay away?

Thanks for any help!
 
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  • #2
Virtual particles cannot be counted, so the rest of your argument kind of goes away.
 

FAQ: Stimulated virtual W+, W- when supernova core-> neutron star?

1. What is a stimulated virtual W+, W- in the context of a supernova core to neutron star transition?

A stimulated virtual W+, W- refers to the creation of virtual particles, specifically charged W bosons, in a highly energetic environment such as a supernova core. These virtual particles are created through quantum fluctuations and play a crucial role in the process of converting a supernova core into a neutron star.

2. How does the presence of stimulated virtual W+, W- affect the supernova core to neutron star transition?

The presence of stimulated virtual W+, W- can greatly impact the dynamics of a supernova core to neutron star transition. These virtual particles can interact with other particles, altering their energy levels and potentially changing the outcome of the transition. Additionally, the creation and annihilation of these virtual particles release energy that can affect the overall energy balance of the system.

3. What is the significance of studying stimulated virtual W+, W- in the context of supernova core to neutron star transitions?

Studying stimulated virtual W+, W- provides insight into the fundamental physics behind the conversion of a supernova core into a neutron star. It also helps researchers better understand the complex dynamics and energy balance involved in this process. Additionally, this research can have implications for our understanding of other high-energy phenomena in the universe.

4. How are stimulated virtual W+, W- detected and measured in a supernova core to neutron star transition?

Stimulated virtual W+, W- cannot be directly detected as they are virtual particles. However, their effects can be observed through their interactions with other particles. For example, the release of energy from the creation and annihilation of these virtual particles can be measured using detectors or telescopes, providing indirect evidence of their presence.

5. Can stimulated virtual W+, W- be manipulated or controlled in a supernova core to neutron star transition?

As virtual particles, stimulated virtual W+, W- cannot be manipulated or controlled in the traditional sense. However, their creation and annihilation can be influenced by changing the conditions of the environment, such as altering the temperature or density of the supernova core. This can indirectly affect the presence and behavior of these virtual particles during the transition process.

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