It looks like you're using an Ad Blocker.
Please white-list or disable AboveTopSecret.com in your ad-blocking tool.
Thank you.
Some features of ATS will be disabled while you continue to use an ad-blocker.
A new study of supermassive black holes at the centers of galaxies has found magnetic fields play an impressive role in the systems’ dynamics. In fact, in dozens of black holes surveyed, the magnetic field strength matched the force produced by the black holes’ powerful gravitational pull, says a team of scientists from the U.S. Department of Energy’s Lawrence Berkeley National Laboratory (Berkeley Lab) and Max Planck Institute for Radio Astronomy (MPIfR) in Bonn, Germany. The findings are published in this week’s issue of Nature.
Tchekhovskoy says the new results mean theorists must re-evaluate their understanding of black-hole behavior. “The magnetic fields are strong enough to dramatically alter how gas falls into black holes and how gas produces outflows that we do observe, much stronger than what has usually been assumed,” he says. “We need to go back and look at our models once again.”
originally posted by: KrzYma
A new study of supermassive black holes at the centers of galaxies has found magnetic fields play an impressive role in the systems’ dynamics. In fact, in dozens of black holes surveyed, the magnetic field strength matched the force produced by the black holes’ powerful gravitational pull, says a team of scientists from the U.S. Department of Energy’s Lawrence Berkeley National Laboratory (Berkeley Lab) and Max Planck Institute for Radio Astronomy (MPIfR) in Bonn, Germany. The findings are published in this week’s issue of Nature.
newscenter.lbl.gov...
hmm.. I thought magnetism is strongly connected to electricity, or is black hole a permanent magnet ?
The material in the accretion disk outside the black hole has spin. An article in 2010 suggested that the 10% of supermassive black holes that have "jets" may have retrograde spin opposite the accretion disk, accounting for the jets, but I think this is still due to the effect it has on the accretion disk:
originally posted by: bbracken677
The earth has a substantial magnetic field due to our spinning core of iron. Perhaps material that falls into a black hole has a significant spin. This would be significant news if true since it has been thought that except for residual radiation that which entered a black hole would not be able to "communicate" outside the black hole.
For two years, Evans has been comparing several dozen galaxies whose black holes host powerful jets (these galaxies are known as radio-loud active galactic nuclei, or AGN) to those galaxies with supermassive black holes that do not eject jets. All black holes — those with and without jets — feature accretion disks, the clumps of dust and gas rotating just outside the event horizon. By examining the light reflected in the accretion disk of an AGN black hole, he concluded that jets may form right outside black holes that have a retrograde spin — or which spin in the opposite direction from their accretion disk. Although Evans and a colleague recently hypothesized that the gravitational effects of black hole spin may have something to do with why some have jets, Evans now has observational results to support the theory in a paper published in the Feb. 10 issue of the Astrophysical Journal.
Since these jets have been shooting out against the gravity of black holes since we first observed them, I'm a little puzzled why the article implies it's any kind of surprise that the magnetic fields are strong. Obviously they have to be some pretty strong fields to accelerate the jets away from the black holes, it shouldn't take a rocket scientists to figure that one out.
The magnetic field strength was confirmed by evidence from jets of gas that shoot away from supermassive black holes.
Well "spin" can mean different things, it can imply a magnetic moment if charged particles are spinning, but some planets without molten cores can rotate on their axes without creating a significant magnetic field and this can also be called spin, but in the "no hair theorem" for black holes, you could remove the ambiguity of this term by calling it "angular momentum".
originally posted by: bbracken677
Therefore, the only way I know of to account for the field strengths would involve spinning the material inside the hole. Previously it was not believed that anything could leave the black hole, but this would suggest that magnetism can.
Gravity can do more than floor you. According to recent measurements of a star system thought to contain a black hole, it can spin you too. This effect, called frame-dragging, is most prominent near massive, fast spinning objects. Now, a team led by W. Cui (MIT) has used the orbiting Rossi X-ray Timing Explorer to search for it near a system thought to contain a black hole. Cui's team claim that matter in this system gets caught up and spun around the black hole at just the rate expected from frame-dragging. Such discoveries help scientists better understand gravity itself.
One of the biggest differences with a black hole as I said earlier is the frame dragging effect. Planets have it too, but Earth's so small it's not that easy to measure and we can say for most practical purposes outside of precise measurements for theory verification, it's probably not significant, especially in relation to the Earth's magnetic field. With black holes, it's much more significant, and there is a model which takes this into account in relation to magnetic fields outside a black hole.
originally posted by: bbracken677
a reply to: Arbitrageur
Aye...I am no astrophysicist, but I am a geologist. I do know how a planet generates it's magnetic field.
As such, drawing a parallel, I proposed that a similar situation may be occurring within the black hole and if so...would it not be unusual in that normally one thinks of the material inside a black hole not being able to "communicate" with the exterior due to the enormous gravity well exerted?
I like the fact you used the qualifier "well" to modify "understood" which IMO makes this statement accurate.
originally posted by: ErosA433
The generation of polar jets is not a well understood process.
The Blandford-Znajek (BZ) process is one of the leading models to explain the launching of powerful relativistic jets emerging from the supermassive black holes at the center of the galaxies (i.e. Active Galactic Nuclei), and the more moderated ones coming from stellar mass black holes (i.e. microquasars). The main ingredients of this process are a central rotating black hole and an accretion disk, which supports a magnetic field threading the black hole horizon. This magnetic field is twisted by the spinning black hole, producing an outgoing electromagnetic flux which extracts energy and angular momentum from the spacetime.
Although the BZ model was introduced a long time ago (R. D. Blandford and R. L. Znajek. (1977)), it is only recently that many issues and theoretical discoveries concerning this mechanism have been settled. These advances on the understanding of the BZ process have been enabled by numerical simulations. For instance, it has been shown that only the magnetic fields lines threading the ergosphere of the black hole (i.e. the region near the black hole where negative killing energies can exist) rotate due to the frame dragging effect, whether or not they cross the horizon
I'm slightly puzzled though because I thought there was previously a problem with models underestimating the jet energy, but that paper actually talks about simulations overestimating the jet energy. I haven't read that last paper yet but it's on my to-do list.
First, we quantify the discrepancies between the BZ jet power and our simulations: assuming maximum efficiency and uniform fields on the horizon leads to a ~10% overestimate of jet power, while ignoring the accretion disk leads to a further ~50% overestimate. Simply reducing the standard BZ jet power prediction by 60% gives a good fit to our simulation data. Our second result is to show that the membrane formulation of the BZ model correctly describes the physics underlying simulated jets: torques, dissipation, and electromagnetic fields on the horizon. This provides intuitive yet rigorous pictures for the black hole energy extraction process. Third, we compute the effective resistance of the load region and show that the load and the black hole achieve near perfect impedance matching. Taken together, these results increase our confidence in the BZ model as the correct description of jets observed from astrophysical black holes.