Exploring the Possibility of Quasars Emitting Above Their Eddington Limit

In summary, a recent study has found that higher redshift quasars are emitting more energy than expected, even beyond their Eddington limit. This may seem counterintuitive as it raises questions about the stability of the accretion disk. However, the study offers a potential explanation for this phenomenon and highlights the limitations of the Eddington limit in its current form.
  • #1
Aziza
190
1
A study is showing that higher redshift quasars emit more and more above their Eddington limit. How is this possible? Shouldnt this be causing the accretion disk to fly apart?
 
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  • #2
Do you have a link to this study?
 
  • #3
Drakkith said:
Do you have a link to this study?

yup here it is!

http://webcache.googleusercontent.com/search?q=cache:1XHScFrhhEYJ:symposia.obs.carnegiescience.edu/series/symposium1/ms/szuszkiewicz_ms.ps.gz+&cd=1&hl=en&ct=clnk&gl=us
 
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  • #4
the study tries to give an explantion .
it has been known for a while that the Eddington Limit(Le) can be exceeded for periods of time..
but recall that the Le is a hypthetical limit based on the presumption that all the material is ionized hydorgen and all the material is accreted uniformally.
 
  • #5


I find this study on the possibility of quasars emitting above their Eddington limit to be very intriguing. The Eddington limit is the theoretical maximum luminosity that an object can emit based on its mass. It is determined by the balance between the inward gravitational force and the outward radiation pressure. Therefore, it is expected that if a quasar emits above its Eddington limit, the accretion disk should fly apart due to the overwhelming radiation pressure.

However, there could be several explanations for the observed trend of higher redshift quasars emitting more above their Eddington limit. One possibility is that these quasars have larger black holes with higher mass accretion rates, which would explain their higher luminosity. Another explanation could be that the Eddington limit itself is not a fixed value and can vary depending on the properties of the accretion disk and the environment of the quasar.

It is also important to consider the limitations of the study and potential sources of error. The redshift measurements of quasars can be affected by various factors such as the Doppler effect and gravitational lensing, which could lead to an overestimation of the quasar's luminosity. Additionally, the Eddington limit is based on theoretical calculations and may not accurately reflect the true limit in extreme environments such as quasars.

In conclusion, while it may seem counterintuitive for quasars to emit above their Eddington limit, further studies and observations are needed to fully understand this phenomenon. It is also important to consider alternative explanations and potential sources of error before drawing definitive conclusions.
 

1. How do quasars emit above their Eddington limit?

Quasars are powered by supermassive black holes at the center of galaxies. As matter falls into the black hole, it releases energy in the form of radiation, causing the quasar to emit light. When the rate of matter falling into the black hole exceeds a certain threshold known as the Eddington limit, the excess energy is released in the form of powerful jets, causing the quasar to emit above its Eddington limit.

2. What is the Eddington limit?

The Eddington limit is a theoretical limit for the maximum amount of radiation that a black hole can emit when it is actively accreting matter. It is determined by the balance between the inward pull of gravity and the outward force of radiation pressure. If the rate of accretion exceeds this limit, the radiation produced by the black hole will push the accreting material away, limiting further growth.

3. How do scientists study the possibility of quasars emitting above their Eddington limit?

Scientists use various telescopes and instruments, such as X-ray telescopes and radio interferometers, to observe and study the properties of quasars. They also analyze the spectra of the emitted radiation to determine the rate of accretion and the energy output of the quasar. This data can then be used to investigate the possibility of quasars emitting above their Eddington limit.

4. What are the implications of quasars emitting above their Eddington limit?

If quasars are indeed emitting above their Eddington limit, it could have significant implications for our understanding of black hole growth and the evolution of galaxies. It may also help explain why some galaxies have extremely bright quasars, while others do not. Additionally, it could provide further insights into the mechanisms behind the formation and behavior of these powerful cosmic objects.

5. Are there any other theories that could explain the high energy output of quasars?

Yes, there are other theories that could potentially explain the high energy output of quasars, such as the presence of a binary black hole system, or the interaction between the accreting material and the magnetic field of the black hole. However, studying the possibility of quasars emitting above their Eddington limit is an important avenue of research that can help us better understand these enigmatic objects and their role in the universe.

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