Not exact matches
The study, «Accretion - induced variability links young stellar objects, white dwarfs, and
black holes», which is published in the journal Science Advances, shows how the «flickering» in the visible brightness of young stellar objects (YSOs)-- very young stars in the final stages of formation — is similar to the flickering seen from
black holes or white dwarfs
as they violently pull matter from their surroundings in a
process known
as accretion.
Four decades ago, he realized that a
black hole's event horizon is inherently leaky; quantum
processes allow a slow but steady flow of particles away from the
black hole, a
process now known
as Hawking radiation.
Supermassive
black holes do the same, and if similar
processes are behind the bursts, watching Cygnus X-3 could tell us how they develop
as they gobble up matter from their surroundings.
The
process of
black hole formation was first described by J. Robert Oppenheimer and Hartland Snyder in the same issue of the Physical Review
as Bohr and Wheeler's fission paper.
The snag is that to run this
process backwards and make the eternal
black hole, you would need to send in a precisely crafted burst of radiation
as the
hole forms.
The
process will likely shrink the small
black holes into an ever - tighter clump around the supermassive
black hole as time goes on, says astrophysicist Abraham Loeb of Harvard University in Cambridge, Massachusetts.
For many aspects of the simulation, researchers can start their calculations at a fundamental, or ab initio, level with no need for preconceived input data, but
processes that are less understood — such
as star formation and the growth of supermassive
black holes — need to be informed by observation and by making assumptions that can simplify the deluge of calculations.
In the early universe, galaxies collided relatively often and their
black holes sometimes merged, growing more massive in the
process and sometimes birthing hugely energetic objects known
as quasars.
Dopita describes the
process as a kind of cosmic indigestion: «It is
as if the
black hole sucks in too much, too quickly, and it burps out gas.»
That
process, now known
as Hawking radiation, explains why we do not have to fear any mini
black holes created by the Large Hadron Collider; they would «evaporate» into radiation almost instantly.
Therefore, the
black hole remnants would be produced at an infinite rate; even such everyday physical
processes as turning on a microwave oven would generate them.
By tracking the positions and properties of hundreds of millions of randomly distributed particles
as they collide and annihilate each other near a
black hole, the new model reveals
processes that produce gamma rays with much higher energies,
as well
as a better likelihood of escape and detection, than ever thought possible.
The concept is a variant of the Penrose
process, first identified in 1969 by British astrophysicist Sir Roger Penrose
as a mechanism for extracting energy from a spinning
black hole.
The merger of two
black holes, such
as the one which produced the gravitational waves discovered by the LIGO Observatory, is considered an extremely complex
process that can only be simulated by the world's most powerful supercomputers.
But a satiated
black hole effectively has zero temperature, barring a trickle of particles released by a
process called Hawking radiation, meaning it could potentially act
as a cold sun, says Opatrný.
The feeding
process is somewhat similar to what happens around supermassive
black holes, but isn't
as big and messy.
In the case of a
black hole in the vicinity of a Schwarzschild sphere there are no stationary potentials
as there is a constant
process of collapse, the boundary of the «
hole» moves away and the energy spectrum is continuous.
It is this twisted field that accelerates particles away from the
black hole as jets and, in the
process, extracts energy from the rotation of the
black hole.
As we noted, the LHC will not destroy the world and as George Musser wrote to me after we recorded the interview, «I said something to the effect that scientists had stocked [stoked] concerns about black holes by saying the LHC would create particles not seen since the big bang, but those particles have been seen since the big bang, namely in natural processes such as cosmic ray collisions; therefore if black holes posed a threat, the universe would already be a goner.&raqu
As we noted, the LHC will not destroy the world and
as George Musser wrote to me after we recorded the interview, «I said something to the effect that scientists had stocked [stoked] concerns about black holes by saying the LHC would create particles not seen since the big bang, but those particles have been seen since the big bang, namely in natural processes such as cosmic ray collisions; therefore if black holes posed a threat, the universe would already be a goner.&raqu
as George Musser wrote to me after we recorded the interview, «I said something to the effect that scientists had stocked [stoked] concerns about
black holes by saying the LHC would create particles not seen since the big bang, but those particles have been seen since the big bang, namely in natural
processes such
as cosmic ray collisions; therefore if black holes posed a threat, the universe would already be a goner.&raqu
as cosmic ray collisions; therefore if
black holes posed a threat, the universe would already be a goner.»
Specifically, the most energetic iron emission they studied is characteristic of so - called x-ray binary starsduos comprised of a dense stellar object such
as a white dwarf star, a neutron star or a
black hole that collects matter from a less dense companion, emitting x-rays in the
process.
After
processing and correlating the data, they will obtain either a glorious silhouette of the
black hole against the brilliant matter swirling around it or,
as in earlier attempts using fewer telescopes, a tantalizing blur.
«This is an indication that the [
black hole] ejection
process is not
as efficient
as we thought.»
If the
black hole has gas or stars to «eat,» that
process generates large amounts of energy
as the infalling gas is compressed and heated to high temperatures.
The
process of converting mass to energy from falling onto a
black hole has an efficiency that is over ten times
as large
as the efficiency of nuclear fusion.
The Expanded VLA will allow scientists to tackle important outstanding questions such
as the formation
processes of stars and planets; the nature of
black holes and the phenomena surrounding them; and the nature of the early universe.
Stephen Hawking theorized in 1974 that
black holes radiate small numbers of particles (mainly photons), a
process known
as «Hawking Radiation».
The DFS highlights three areas of particular concern: ensuring payments are
processed quickly to build user confidence that money will not «get stuck in a digital
black hole»; ensuring virtual currencies do not become the tool of choice for terrorists, drug smugglers, illegal weapons dealers, money launderers, and human traffickers; making sure that the use of bitcoin
as an investment is governed properly.
I have often heard job seekers refer to the application
process as a «
black hole where resumes go, never to be heard from again».