«We can't avoid the conclusions that
they really are black holes,» Heyl says.
If there
really were a black hole between us and Boyajian's star, we would expect a brightening, not dimming, which we definitely do not see.
Although this might seem like an excellent source of job leads, it can
really be a black hole due to the amount of competition and resume submissions.
Not exact matches
In other words, a properly ordered will (one that leads toward good things in good measure) following closely on the heels of right reason (one that perceives and presents to the will goods
really perfective of the human person) goes a long way to putting the passions in their place (which
is not, emphatically, squashed way down into a virtual
black hole).
If you
really care that much, it
's not hard to test, mass
is directly proportional to gravitational strength, I told you how far the
black hole is, and alpha centarui
is about 4 lightyears away.
So they
're kind of the same in some deep mathematical sense, and as of today we don't
really know what happens at the center of a
black hole and we don't
really know what happened at the moment of the big bang so these
are two puzzles that
are cousins of one another and anything that we learn about one
is certainly going to shed light on the other.»
«With private label, I did not have to spend the money needed to build a brand, which
really can
be a
black hole,» he explains.
And I
'm not
really sure where the money goes, into a
black hole never to
be seen again for the most part so I
'm happy to keep as much as possible.
The idea of matter escaping the alleged point - of - no - return
was surprising (it
's a central plot point in that other recent movie about
black holes, the biographical The Theory of Everything), but the fate of information that falls into the
black hole was what
really troubled Hawking
's colleagues.
«Where this model
really shines
is explaining the late emission,» says Chris Fryer of Los Alamos National Laboratory in New Mexico — one of the physicists who first proposed the burrowing
black hole theory in the 1990s.
To study co-author Krzystof Stanek, the
really interesting part of the discovery
is the implications it holds for the origins of very massive
black holes — the kind that the LIGO experiment detected via gravitational waves.
«It
's really hard to torque a
black hole around by a large amount without having something as massive as another
black hole slam into it,» says astrophysicist Scott Hughes of the University of California, Santa Barbara, co-author of a forthcoming independent analysis that draws similar conclusions.
Theoretical physicists spent decades demonstrating that
black holes really were consistent with Einstein's ideas and working out how they should behave.
And the reason you can get energy out of a
black hole, that swallower of all things,
is that the energy you detect never
really got into the
black hole to begin with — it
's associated with the space - time whirlpool created outside the event horizon by the
black hole's rotation.
HAWKING»S LEGACY Among Stephen Hawking's most notable contributions to physics
was the discovery that
black holes are not
really black.
A
black hole really is an object with very rich structure, just like Earth has a rich structure of mountains, valleys, oceans, and so forth.
Is it
really a
black hole?
Being someone who knows the tip of the iceberg about things like
black holes, it
's really mind - boggling to read the works and findings of brilliant scientists in such a comprehensible way.
«It
's the first time that general relativity
is really tested around a supermassive
black hole,» says Aurélien Hees at the University of California, Los Angeles.
It
is a region of space where you have mass that
's confined to zero volume, which means that the density
is infinitely large, which means we have no way of describing,
really, what a
black hole is!
I think the question
really is about our description of the physical world, as opposed to the matter content of the
black hole.
One of the most important scientific consequences of detecting a
black -
hole merger would
be confirmation that
black holes really do exist — at least as the perfectly round objects made of pure, empty, warped space - time that
are predicted by general relativity.
However, researchers
are still not sure it
's really a
black hole.
And the reason you can getenergy out of a
black hole, that swallower of all things,
is that theenergy you detect never
really got into the
black hole to beginwith — it
's associated with the space - time whirlpool created outside theevent horizon by the
black hole's rotation.
Ray Jayawardhana: It
is a clue that most likely, these high energy neutrinos come either from jets of particles that
are accelerated by super massive
black holes at the hearts of galaxies, or from
really gigantic stars that explode at the end of their lives that also produce a phenomenon we call gamma ray bursts, which also might accelerate particles to very high speeds and energies.
Even protostars — these
are young stars that
are just forming and making their own planetary disks and so on — they make very powerful outflows called, the same sort of jets obviously moving at slower speeds, but they
are full of plasma, that
is flowing out at high speed; white dwarfs, neutron stars,
black holes big and small, they seem able to do this task, it
really seems to
be a very common phenomenon.
«Our motive
is not so much to establish that there
is a hard surface,» Kumar said, «but to push the boundary of knowledge and find concrete evidence that
really, there
is an event horizon around
black holes.»
Supermassive
black holes in the cores of galaxies
are thought to fatten slowly over eons, so finding such a heavyweight so early in the history of the universe
is «
really pushing it,» he says.
«Using measurements that
were done at BYU, we
were able to determine that the mass of the central
black hole for this galaxy
was about 8 million times the mass of the sun — that
's a
really really massive object.»
«It will
be really exciting to compare the results with the evolution of galaxies, given the close links between
black hole and galaxy formation,» says Willott.
Then he explains that
black holes — and quarks and gluons —
are really no stranger than a cup of water.
Son insists that
black holes, quarks, and gluons
really do have a big thing in common: They can
be described by equations that govern the behavior of liquids.
So the very hot quarks and gluons at RHIC may
really be a hologram of some nasty
black hole somewhere.»
But it makes it sound like it
's a 50 — 50 shot and some of the press attention to the collider
is dwelling on the possibility of the creation of these mini
black holes that could become, that could grow and, you know, destroy the entire planet, solar system, but so why don't we talk just from all around why that
's really press sensationalism.
«It would
be really wonderful if the
black hole were cataclysmic now,» he sighs.
Unfortunately, there
's no good way to study a
black hole up close to test what
's really going on.
«To change in brightness, you have to
be a small object, and that
really narrows it down to a
black hole,» he says.
Such isolated
black holes would
be too dim to discern at the galactic core, but the x-ray binaries serve as a tracer suggesting they
're there — and in
really big numbers.
Other theories, like mergers of smaller
black holes, remain viable, and researchers aren't quite sure yet how many
black holes there
really are in the early universe.
«It
is, I think, the clearest indication that
black holes are really there,» says Penrose.
The alternative
is that the stars
really are young, but how you get stars to form that close to the
black hole is very difficult.
It
's tough to describe
black -
hole spin rates because they don't
really translate into familiar terms, such as miles per hour.
But how will scientists
be really sure that there
is a
black hole in our Milky Way and not something else that behaves in a very similar way?
«Astrophysicists have
been collecting observational evidence for both stellar mass
black holes and supermassive
black holes for decades, but even though we think the largest ones grow from the smallest ones, we've never
really had clear evidence for a
black hole with a mass in between those extremes,» she added.
«However, a lot of work remains to
be done to test whether this idea will actually pan out; this
is really just the tip of the iceberg in terms of realistic simulations of
black holes in the early universe.»
And what that
really means
is the ringing of space sweeps up in frequency as the
black holes get faster and faster and finally merge.
Only polarization of Sgr A * light permits to constrain the geometry of the magnetic fields near the
black hole event horizon and it
is possibly the only way to find out what Sgr A * radio source
really is.
The waves, first predicted by Albert Einstein roughly a century ago,
are basically ripples in the fabric of space - time caused by the acceleration of
really massive objects such as
black holes.
«For some people, seeing
really is believing, so we
were hoping to get something in time,» said Shep Doeleman, an astronomer at the Harvard - Smithsonian Center for Astrophysics who
is leading the effort to photograph a
black hole, known as the Event Horizon Telescope, or EHT.
«I thought this idea of growing a massive star in a special configuration and forming a
black hole with the right kind of masses
was something we could approximate, but to see the
black hole inducing star formation and driving the dynamics in ways that we've observed in nature
was really icing on the cake.»