Tag Archives: Black

Swirling Vortex of Bathtub Water Reveals an Elusive Mechanism of Black Hole Physics

When a black hole is active, we tend to focus on the effect it has on the material it’s slurping up. It makes sense to do so; black holes themselves are difficult to probe. But the interaction between the black hole and the material should have an effect on the black hole, too – as it gains material, it should also gain in mass.

 

Such small feedback responses – especially ones previously ignored as trivial – are known as backreactions, and scientists have just observed an analogue of one that’s specific to black holes, and which can be seen in water swirling down a drain.

It’s a detection that could help study black hole phenomena that are too subtle for our current instruments, such as the Hawking radiation that is thought to be emitted by black holes. This is a theoretical type of black-body radiation that would eventually – after a very, very long time – see a black hole completely evaporate, provided it was not growing at all.

In order to study cosmic objects in finer detail than we can across the vast distances of space, scaled-down versions, or analogues, can be created in a lab. Like, for instance, a recent experiment to replicate white dwarf core pressures.

Black hole analogues are an excellent way to find out more about these enigmatic objects, and different kinds can help reveal their secrets in multiple ways.

Optical fibre and Bose-Einstein condensates have both been used to learn more about Hawking radiation. But one of the simplest has to do with how black holes feed: the draining bathtub vortex.

 

Black hole accretion can be compared with water swirling down a drain. Treating matter as a ripple in a field, the water can stand in for spacetime itself, or a field rippling with quantum activity.

Measuring the ripples responses as the water vanishes down a swirling drain might have something to say about waves of energy disappearing into a black hole.

A bathtub vortex black hole analogue. (The University of Nottingham)

From such analogues, we’ve learnt a lot about the effect of black holes on the space and material around them. But with an external water pump keeping the background of the system steady, it was unclear whether a water black hole analogue would have the freedom to be able to react to waves.

This set of experiments is the first time a draining bathtub vortex has demonstrated an effect on the black hole itself.

“We have demonstrated that analogue black holes, like their gravitational counterparts, are intrinsically backreacting systems,” said physicist Sam Patrick of the University of Nottingham in the UK.

“We showed that waves moving in a draining bathtub push water down the plug hole, modifying significantly the drain speed and consequently changing the effective gravitational pull of the analogue black hole.”

 

When waves were sent rippling into the system towards the drain, they pushed extra water in, accelerating the “accretion” process so significantly that the water levels in the tub dropped noticeably, even while a pump maintained the same level of water going in.

This change in the water level corresponds to a change in the properties of the black hole, the researchers said.

This could be extremely useful information, partially because an increase in mass changes the gravitational strength of a black hole – it changes the way the black hole warps its surrounding spacetime, as well as the effect the black hole has on the accretion disc. In addition, it offers a new way to study how waves can affect black hole dynamics.

“What was really striking for us is that the backreaction is large enough that it causes the water height across the entire system to drop so much that you can see it by eye! This was really unexpected,” Patrick said.

“Our study paves the way to experimentally probing interactions between waves and the spacetimes they move through. For example, this type of interaction will be crucial for investigating black hole evaporation in the laboratory.”

The team’s research has been published in Physical Review Letters.

 

Read original article here

There Is One Way Humans Could ‘Safely’ Enter a Black Hole, Physicists Say

To solve the mysteries of black holes, a human should just venture into one.

However, there is a rather complicated catch: A human can do this only if the respective black hole is supermassive and isolated, and if the person entering the black hole does not expect to report the findings to anyone in the entire Universe.

 

We are both physicists who study black holes, albeit from a very safe distance. Black holes are among the most abundant astrophysical objects in our Universe.

These intriguing objects appear to be an essential ingredient in the evolution of the Universe, from the Big Bang till present day. They probably had an impact on the formation of human life in our own galaxy.

A person falling into a black hole and being stretched. (Leo Rodriguez/Shanshan Rodriguez/CC BY-ND)

Two types of black holes

The Universe is littered with a vast zoo of different types of black holes.

They can vary by size and be electrically charged, the same way electrons or protons are in atoms. Some black holes actually spin. There are two types of black holes that are relevant to our discussion.

The first does not rotate, is electrically neutral – that is, not positively or negatively charged – and has the mass of our Sun. The second type is a supermassive black hole, with a mass of millions to even billions times greater than that of our Sun.

Besides the mass difference between these two types of black holes, what also differentiates them is the distance from their center to their “event horizon” – a measure called radial distance.

A person falling into a supermassive black hole would likely survive. (Leo & Shanshan Rodriguez/CC BY-ND)

The event horizon of a black hole is the point of no return. Anything that passes this point will be swallowed by the black hole and forever vanish from our known Universe.

At the event horizon, the black hole’s gravity is so powerful that no amount of mechanical force can overcome or counteract it. Even light, the fastest-moving thing in our Universe, cannot escape – hence the term “black hole”.

The radial size of the event horizon depends on the mass of the respective black hole and is key for a person to survive falling into one. For a black hole with a mass of our Sun (one solar mass), the event horizon will have a radius of just under 2 miles (3.2 kilometres).

A person approaching the event horizon of a a Sun-size black hole. (Leo and Shanshan Rodriguez/CC BY-ND)

The supermassive black hole at the center of our Milky Way galaxy, by contrast, has a mass of roughly 4 million solar masses, and it has an event horizon with a radius of 7.3 million miles or 17 solar radii.

Thus, someone falling into a stellar-size black hole will get much, much closer to the black hole’s center before passing the event horizon, as opposed to falling into a supermassive black hole.

 

This implies, due to the closeness of the black hole’s center, that the black hole’s pull on a person will differ by a factor of 1,000 billion times between head and toe, depending on which is leading the free fall.

In other words, if the person is falling feet first, as they approach the event horizon of a stellar mass black hole, the gravitational pull on their feet will be exponentially larger compared to the black hole’s tug on their head.

The person would experience spaghettification, and most likely not survive being stretched into a long, thin noodle-like shape.

Now, a person falling into a supermassive black hole would reach the event horizon much farther from the the central source of gravitational pull, which means that the difference in gravitational pull between head and toe is nearly zero.

Thus, the person would pass through the event horizon unaffected, not be stretched into a long, thin noodle, survive and float painlessly past the black hole’s horizon.

Other considerations

Most black holes that we observe in the Universe are surrounded by very hot disks of material, mostly comprising gas and dust or other objects like stars and planets that got too close to the horizon and fell into the black hole.

These disks are called accretion disks and are very hot and turbulent. They are most certainly not hospitable and would make traveling into the black hole extremely dangerous.

 

To enter one safely, you would need to find a supermassive black hole that is completely isolated and not feeding on surrounding material, gas, or even stars.

Now, if a person found an isolated supermassive black hole suitable for scientific study and decided to venture in, everything observed or measured of the black hole interior would be confined within the black hole’s event horizon.

Keeping in mind that nothing can escape the gravitational pull beyond the event horizon, the in-falling person would not be able to send any information about their findings back out beyond this horizon. Their journey and findings would be lost to the rest of the entire Universe for all time. But they would enjoy the adventure, for as long as they survived … maybe ….

Leo Rodriguez, Assistant Professor of Physics, Grinnell College and Shanshan Rodriguez, Assistant Professor of Physics, Grinnell College.

This article is republished from The Conversation under a Creative Commons license. Read the original article.

 

Read original article here

Seattle Public Schools’ Black Lives Matter lesson plans advance ‘anti-police narratives’: radio host

Seattle Public Schools teaching Black Lives Matter lesson plans to children advance “anti-police narratives,” radio host Jason Rantz said on Tuesday.

“This is a curriculum that, to be clear, doesn’t just impact Seattle. This is happening all across the country this week in schools,” the radio talk show of KTTH Seattle told “The Faulkner Focus.” 

The Black Lives Matter curriculum-integrated program teaches students explicitly how to become progressive social justice activists, among other things.

“It forwards a number of anti-police narratives, including that police purposely target African Americans with the intent to kill, that they choose not to de-escalate, that they are quick to use force because of their training,” Rantz said.

LAID-OFF KEYSTONE XL WORKER SAYS DECISION TO CANCEL PIPELINE ‘IS GOING TO HURT A LOT OF PEOPLE’

Black Lives Matter lesson plans are “radical,” Rantz argued in an article he wrote on Tuesday.

Seattle Public Schools are conducting a “Black Lives Matter at School Week” that runs Feb. 1 through Feb. 5. 

Rantz wrote, “It indoctrinates elementary- and middle-schoolers into believing that Black people are ‘systematically and intentionally targeted for demise’ in this country. They even learn to blame and distrust the police.”

“There isn’t a hint of ideological diversity in any of the lesson plans,” Rantz said.

Blasting the content being taught to students, Rantz said that the curriculum calls “any jail or immigration law state violence.”

CLICK HERE TO GET THE FOX NEWS APP

“And it doesn’t just stop on policing and issues of diversity,” Rantz said. “It specifically says that it’s going after the family structure. It teaches kids as young as kindergartners that they should be choosing their own gender. And I think my favorite line from some of the curriculum that was put out there was treating everyone the same might be unintentionally oppressive.”

Read original article here

Backreaction observed for first time in water tank black hole simulation

Lab experiment using water tank simulation to demonstrate backreaction. Credit: University of Nottingham

Scientists have revealed new insights into the behavior of black holes with research that demonstrates how a phenomenon called backreaction can be simulated.

The team from the University of Nottingham have used their simulation of a black hole, involving a specially designed water tank, for this latest research published in Physical Review Letters. This study is the first to demonstrate that the evolution of black holes resulting from the fields surrounding them can be simulated in a laboratory experiment.

The researchers used a water tank simulator consisting of a draining vortex, like the one that forms when you pull the plug in the bath. This mimics a black hole since a wave which comes too close to the drain gets dragged down the plug hole, unable to escape. Systems like these have grown increasingly popular over the past decade as a means to test gravitational phenomena in a controlled laboratory environment. In particular, Hawking radiation has been observed in an analog black hole experiment involving quantum optics.

Using this technique the researchers showed for the first time that when waves are sent into an analog black hole, the properties of the black hole itself can change significantly. The mechanism underlying this effect in their particular experiment has a remarkably simple explanation. When waves come close to the drain, they effectively push more water down the plug hole causing the total amount of water contained in the tank to decrease. This results in a change in the water height, which in the simulation corresponds to a change in the properties of the black hole.

Lead author, Post-doctoral researcher Dr. Sam Patrick from the University of Nottingham School of Mathematical Sciences explains: “For a long time, it was unclear whether the backreaction would lead to any measurable changes in analog systems where the fluid flow is driven, for example, using a water pump. We have demonstrated that analog black holes, like their gravitational counterparts, are intrinsically backreacting systems. We showed that waves moving in a draining bathtub push water down the plug hole, modifying significantly the drain speed and consequently changing the effective gravitational pull of the analog black hole.

What was really striking for us is that the backreaction is large enough that it causes the water height across the entire system to drop so much that you can see it by eye! This was really unexpected. Our study paves the way to experimentally probing interactions between waves and the spacetimes they move through. For example, this type of interaction will be crucial for investigating black hole evaporation in the laboratory.”

Black hole research at the University of Nottingham has recently received a £4.3 million funding boost for a three-year project that aims to provide further insights into the physics of the early universe and black holes.

The research team will use quantum simulators to mimic the extreme conditions of the early universe and black holes. The Nottingham team will be using a new state laboratory to set up a novel hybrid superfluid optomechanical system to mimic quantum black hole processes in the laboratory.


Black holes gain new powers when they spin fast enough


More information:
Sam Patrick et al, Backreaction in an Analogue Black Hole Experiment, Physical Review Letters (2021). DOI: 10.1103/PhysRevLett.126.041105
Provided by
University of Nottingham

Citation:
Backreaction observed for first time in water tank black hole simulation (2021, February 1)
retrieved 1 February 2021
from https://phys.org/news/2021-02-backreaction-tank-black-hole-simulation.html

This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no
part may be reproduced without the written permission. The content is provided for information purposes only.



Read original article here

Could a human enter a black hole to study it?

A person falling into a black hole and being stretched while approaching the black hole’s horizon. Leo Rodriguez and Shanshan Rodriguez, CC BY-ND” src=”https://s.yimg.com/ny/api/res/1.2/SBvGJ3rPz3b8fjBD17Qscw–/YXBwaWQ9aGlnaGxhbmRlcjt3PTcwNTtoPTI0Ni4yNjA0MTY2NjY2NjY2Ng–/https://s.yimg.com/uu/api/res/1.2/D.mRPFzroWLnC_dpHzf0Og–~B/aD01MDM7dz0xNDQwO2FwcGlkPXl0YWNoeW9u/https://media.zenfs.com/en/the_conversation_us_articles_815/42c590c6ac2b6823773318ce894066df” data-src=”https://s.yimg.com/ny/api/res/1.2/SBvGJ3rPz3b8fjBD17Qscw–/YXBwaWQ9aGlnaGxhbmRlcjt3PTcwNTtoPTI0Ni4yNjA0MTY2NjY2NjY2Ng–/https://s.yimg.com/uu/api/res/1.2/D.mRPFzroWLnC_dpHzf0Og–~B/aD01MDM7dz0xNDQwO2FwcGlkPXl0YWNoeW9u/https://media.zenfs.com/en/the_conversation_us_articles_815/42c590c6ac2b6823773318ce894066df”/>
A person falling into a black hole and being stretched while approaching the black hole’s horizon. Leo Rodriguez and Shanshan Rodriguez, CC BY-ND

Curious Kids is a series for children of all ages. If you have a question you’d like an expert to answer, send it to CuriousKidsUS@theconversation.com.

Could a human enter a black hole to study it? – Pulkeet, age 12, Bahadurgarh, Haryana, India

To solve the mysteries of black holes, a human should just venture into one. However, there is a rather complicated catch: A human can do this only if the respective black hole is supermassive and isolated, and if the person entering the black hole does not expect to report the findings to anyone in the entire universe.

We are both physicists who study black holes, albeit from a very safe distance. Black holes are among the most abundant astrophysical objects in our universe. These intriguing objects appear to be an essential ingredient in the evolution of the universe, from the Big Bang till present day. They probably had an impact on the formation of human life in our own galaxy.

Two types of black holes

The universe is littered with a vast zoo of different types of black holes.

They can vary by size and be electrically charged, the same way electrons or protons are in atoms. Some black holes actually spin. There are two types of black holes that are relevant to our discussion. The first does not rotate, is electrically neutral – that is, not positively or negatively charged – and has the mass of our Sun. The second type is a supermassive black hole, with a mass of millions to even billions times greater than that of our Sun.

Besides the mass difference between these two types of black holes, what also differentiates them is the distance from their center to their “event horizon” – a measure called radial distance. The event horizon of a black hole is the point of no return. Anything that passes this point will be swallowed by the black hole and forever vanish from our known universe.

At the event horizon, the black hole’s gravity is so powerful that no amount of mechanical force can overcome or counteract it. Even light, the fastest-moving thing in our universe, cannot escape – hence the term “black hole.”

The radial size of the event horizon depends on the mass of the respective black hole and is key for a person to survive falling into one. For a black hole with a mass of our Sun (one solar mass), the event horizon will have a radius of just under 2 miles.

The supermassive black hole at the center of our Milky Way galaxy, by contrast, has a mass of roughly 4 million solar masses, and it has an event horizon with a radius of 7.3 million miles or 17 solar radii.

Thus, someone falling into a stellar-size black hole will get much, much closer to the black hole’s center before passing the event horizon, as opposed to falling into a supermassive black hole.

This implies, due to the closeness of the black hole’s center, that the black hole’s pull on a person will differ by a factor of 1,000 billion times between head and toe, depending on which is leading the free fall. In other words, if the person is falling feet first, as they approach the event horizon of a stellar mass black hole, the gravitational pull on their feet will be exponentially larger compared to the black hole’s tug on their head.

The person would experience spaghettification, and most likely not survive being stretched into a long, thin noodlelike shape.

Now, a person falling into a supermassive black hole would reach the event horizon much farther from the the central source of gravitational pull, which means that the difference in gravitational pull between head and toe is nearly zero. Thus, the person would pass through the event horizon unaffected, not be stretched into a long, thin noodle, survive and float painlessly past the black hole’s horizon.

Other considerations

Most black holes that we observe in the universe are surrounded by very hot disks of material, mostly comprising gas and dust or other objects like stars and planets that got too close to the horizon and fell into the black hole. These disks are called accretion disks and are very hot and turbulent. They are most certainly not hospitable and would make traveling into the black hole extremely dangerous.

To enter one safely, you would need to find a supermassive black hole that is completely isolated and not feeding on surrounding material, gas and or even stars.

Now, if a person found an isolated supermassive black hole suitable for scientific study and decided to venture in, everything observed or measured of the black hole interior would be confined within the black hole’s event horizon.

Keeping in mind that nothing can escape the gravitational pull beyond the event horizon, the in-falling person would not be able to send any information about their findings back out beyond this horizon. Their journey and findings would be lost to the rest of the entire universe for all time. But they would enjoy the adventure, for as long as they survived … maybe ….

Hello, curious kids! Do you have a question you’d like an expert to answer? Ask an adult to send your question to CuriousKidsUS@theconversation.com. Please tell us your name, age and the city where you live.

And since curiosity has no age limit – adults, let us know what you’re wondering, too. We won’t be able to answer every question, but we will do our best.

This article is republished from The Conversation, a nonprofit news site dedicated to sharing ideas from academic experts. It was written by: Leo Rodriguez, Grinnell College and Shanshan Rodriguez, Grinnell College.

Read more:

The authors do not work for, consult, own shares in or receive funding from any company or organization that would benefit from this article, and have disclosed no relevant affiliations beyond their academic appointment.

Read original article here

A Louisiana cemetery told the family of a Black deputy he couldn’t be buried there because it was only for White people

Her husband Darrell Semien, a sheriff’s deputy for Allen Parish, Louisiana, died on January 24 after being diagnosed with cancer in December, CNN affiliate KPLC reported.

Semien went to Oaklin Springs Cemetery in Oberlin earlier this week to inquire about laying her husband to rest there. But a woman at the cemetery turned her away because her husband was African American.

“I met with the lady out there and she said she could NOT sell me a plot because the cemetery is a WHITES ONLY cemetery,” Semien wrote on Facebook. “She even had paperwork on a clipboard showing me that only white human beings can be buried there. She stood in front of me and all my kids. Wow what a slap in the face.”

CNN has reached out to Semien for comment.

Creig Vizena, president of the Oaklin Springs Cemetery Association, told CNN affiliate KATC that he was ashamed to learn about how the Semien family had been treated. The woman who turned them away was in her 80s and has since been “relieved of her duties,” he told the Washington Post.

CNN was unable to reach Vizena for comment.

Vizena told KPLC that he hadn’t been aware of the language contained in the cemetery’s sales contracts, which date back to the 1950s and included the phrase “the right of burial of the remains of white human beings.” The issue hadn’t come up before, he said.

“I take full responsibility for that,” Vizena told KPLC. “I’ve been the president of this board for several years now. I take full responsibility for not reading the by-laws.”

Board members of the cemetery held an emergency meeting on Thursday to remove the clause from the contract, KPLC reported.

Vizena apologized and said he offered the family one of the plots that he owns so that Darrell Semien could be buried there. But the damage had been done, and they declined.

Segregated cemeteries have a long history in the US, and remnants from those dark chapters persist to this day.

In 2016, the city of Waco, Texas, ordered the removal of a chain-link fence from a public cemetery that was used to separate the White section from the Black section. A similar fence at a cemetery in Mineola, Texas, came down last year.

The ACLU of Louisiana urged the Oaklin Springs Cemetery Association to remove any “Whites only” references from its bylaws, citing the Supreme Court’s 1948 decision in Shelley v. Kraemer that outlawed racial covenants in housing.

“It is unconscionable and unacceptable that the Semien family—or anyone else—should face such blatant racial discrimination, especially during a time of mourning and grief,” the organization wrote in a letter.

Read original article here

Extreme black holes have hair that can be combed

Artist’s conception of a rotating black hole accreting matter via an accretion disk and emitting a jet. Credit: NASA/JPL-Caltech

Black holes are considered amongst the most mysterious objects in the universe. Part of their intrigue arises from the fact that they are actually among the simplest solutions to Einstein’s field equations of general relativity. In fact, black holes can be fully characterized by only three physical quantities: their mass, spin and charge. Since they have no additional “hairy” attributes to distinguish them, black holes are said to have “no hair”—Black holes of the same mass, spin, and charge are exactly identical to each other.

Dr. Lior Burko of Theiss Research in collaboration with Professor Gaurav Khanna of the University of Massachusetts Dartmouth and the University of Rhode Island alongside his former student Dr. Subir Sabharwal discovered that a special kind of black hole violates black hole uniqueness, the so-called “no hair” theorem. Specifically, the team studied extremal black holes—holes that are “saturated” with the maximum charge or spin they can possibly carry. They found that there is a quantity that can be constructed from the spacetime curvature at the black hole horizon that is conserved, and measurable by a distant observer. Since this quantity depends on how the black hole was formed, and not just on the three classical attributes, it violates black hole uniqueness.

This quantity constitutes “gravitational hair” and potentially measurable by recent and upcoming gravitational wave observatories like LIGO and LISA. The structure of this new hair follows the development of a similar quantity that was found by Angelopoulos, Aretakis, and Gajic in the context of a simpler “toy” model using a scalar field and spherical black holes, and extends it to gravitational perturbations of rotating ones.

“This new result is surprising,” said Burko, “because the black hole uniqueness theorems are well established, and in particular their extension to extreme black holes. There has to be an assumption of the theorems that is not satisfied, to explain how the theorems do not apply in this case.” Indeed, the team followed on previous work by Aretakis, that found that even though external perturbations of extreme black holes decay as they do also for regular black holes, along the event horizon certain perturbation fields evolve in time indefinitely. “The uniqueness theorems assume time independence. But the Aretakis phenomenon explicitly violates time independence along the event horizon. This is the loophole through which the hair can pop out and be combed at a great distance by a gravitational wave observatory,” said Burko. Unlike other work that found hair in black hole scalarization, Burko noted that “in this work we were working with the vacuum Einstein theory, without additional dynamical fields that modify the theory and which may violate the Strong Equivalence Principle.”

The team used very intensive numerical simulations to generate their results. The simulations involved using dozens of the highest-end Nvidia graphics-processing-units (GPUs) with over 5,000 cores each, in parallel. “Each of these GPUs can perform as many as 7 trillion calculations per second; however, even with such computational capacity the simulations look many weeks to complete,” said Khanna.


Nearly extreme black holes which attempt to regrow hair become bald again


More information:
Lior M. Burko et al, Scalar and gravitational hair for extreme Kerr black holes, Physical Review D (2021). DOI: 10.1103/PhysRevD.103.L021502

Provided by
Theiss Research

Citation:
Extreme black holes have hair that can be combed (2021, January 26)
retrieved 26 January 2021
from https://phys.org/news/2021-01-extreme-black-holes-hair.html

This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no
part may be reproduced without the written permission. The content is provided for information purposes only.



Read original article here

Microsoft, BlackBerry, GE, Leon Black – 5 Things You Must Know

Here are five things you must know for Tuesday, Jan. 26:

1. — Stock Futures Move Higher on Solid Earnings

Stock futures moved mostly higher Tuesday following solid earnings reports from Johnson & Johnson  (JNJ) – Get Report, 3M  (MMM) – Get Report and General Electric  (GE) – Get Report.

Equities had wavered for most of the premarket session on the possibility that a U.S. coronavirus relief package could be delayed. 

Contracts linked to the Dow Jones Industrial Average rose 56 points, S&P 500 futures rose 2 points and Nasdaq futures were down 7 points ahead of earnings reports from some of the biggest tech companies.

Senate Majority Leader Chuck Schumer said Monday an aid package was unlikely before mid-March. That is when federal unemployment benefits authorized by last $900 billion package will expire.

President Joe Biden said he was open to negotiations on his proposed $1.9 trillion plan to send $1,400 to most Americans and deliver other support for the economy, including funds for vaccine distribution.

A bipartisan group of senators already have voiced opposition to the size of Biden’s plan.

The coronavirus pandemic, meanwhile, has killed more than 421,000 in the U.S. and concerns have been growing about the bumpy rollout of vaccines in the country. Biden said he anticipates vaccines will be available to anyone in the U.S. by spring, but to meet that projection vaccine makers will have to sharply increase production.

Stocks finished mixed on Monday amid questions about whether the Biden White House will be able to deliver another round of stimulus. The S&P 500 and Nasdaq, however, did manage to close at record highs.

2. — Tuesday’s Calendar: Microsoft and AMD Earnings, Federal Reserve Meeting

General Electric  (GE) – Get Report reported fourth-quarter adjusted earnings of 8 cents a share, 1 cent below analysts’ estimates. Total revenue of $21.93 billion topped forecasts.

Johnson & Johnson  (JNJ) – Get Report posted stronger-than-expected fourth- quarter earnings and said Tuesday it would provide an update on its vaccine development progress “soon.”

“We continue to progress our Covid-19 vaccine candidate and look forward to sharing details from our Phase 3 study soon. Johnson & Johnson was built for times like these, and I am extremely confident in our ability to deliver lasting value and continued innovation in 2021 and for years to come,” said CEO Alex Gorsky.

Earnings reports are also expected Tuesday from Microsoft  (MSFT) – Get Report, Advanced Micro Devices  (AMD) – Get Report, Starbucks  (SBUX) – Get Report, Verizon  (VZ) – Get Report, Lockheed Martin  (LMT) – Get Report, American Express  (AXP) – Get Report, 3M  (MMM) – Get Report, Xilinx  (XLNX) – Get Report, Raytheon Technologies  (RTX) – Get Report and Texas Instruments  (TXN) – Get Report.

Microsoft, Advanced Micro Devices and Starbucks are holdings in Jim Cramer’s Action Alerts PLUS member club. Want to be alerted before Jim Cramer buys or sells the stocks? Learn more now.

The U.S. economic calendar on Tuesday includes the first day of a two-day meeting of the Federal Reserve. The central bank isn’t expected to move on interest rates and has signaled it will keep them near zero through 2023.

Mark Heppenstall, chief investment officer at Penn Mutual Asset Management, said the central bank likely will reiterate its “commitment to prolonged monetary accommodation” at the meeting.

“Uncertainty surrounding the pandemic’s near-term course and signs of weakening labor markets suggest recent taper talk by Fed officials is still premature,” Heppenstall added, referring to when the Fed might  begin tapering asset purchases.

The calendar also includes the Case-Shiller Home Price Index for November at 9 a.m. ET and Consumer Confidence for January at 10 a.m.

3. — Leon Black Will Step Down as CEO of Private-Equity Giant Apollo

Leon Black, the founder and CEO of private-equity giant Apollo Global Management  (APO) – Get Report, will step down as chief executive after it was revealed he made larger-than-expected payments to Jeffrey Epstein, the disgraced financier.

Black paid Epstein $158 million in fees for trust- and estate-tax planning in the five years to 2017, far more than was previously known, according to a report from law firm Dechert. 

The review by Dechert found no evidence that Black was involved in the criminal activities of the late Epstein, who was indicted in 2019 on federal sex-trafficking charges involving underage girls. Epstein committed suicide in prison while awaiting child sex charges.

Apollo also never retained Epstein for any services, the report concluded. 

Black wrote in a letter to Apollo’s fund investors that he would cede the role of CEO to co-founder Marc Rowan on or before his 70th birthday on July 31, while retaining the role of chairman. 

The Wall Street Journal was first to report on the contents of the report and letter.

Shares of Apollo Global rose 3.86% to $47.65 in after-hours trading on Monday.

4. — BlackBerry Shares Surge Again

BlackBerry  (BB) – Get Report was jumping more than 11% in premarket trading Tuesday, following the stock’s more than 28% gain in the previous session as it received a boost from retail traders and was being heavily mentioned on online message boards such as Reddit.

BlackBerry, the security software and services company, said in a statement that it was unaware of reasons for the stock move.

Shares of BlackBerry rose 11.87% to $20.17 in premarket trading Tuesday. The stock has gained 172% so far in 2021.

BlackBerry Rises Again, Gets Lift From Expanded Baidu Partnership

Analysts at RBC cut the stock to underperform from sector perform, citing valuation and saying there has been no change to the company’s fundamental outlook. Analyst Paul Treiber maintained his price target at $7.50.

BlackBerry has become a favorite on the Reddit message board, much like GameStop  (GME) – Get Report and Express  (EXPR) – Get Report.

What Is Happening to GameStop Stock? Jim Cramer Explains

5. — Apple Lead Hardware Engineer Shifting to ‘New Project’

Apple  (AAPL) – Get Report said its leading hardware engineer, Dan Riccio, was moving to a new project and will be replaced by John Ternus, currently a vice president of hardware engineering.

Riccio has been with Apple since 1998 and has worked on most of the company’s major products over that time, from the first iMac computers to the latest 5G phones.

Apple didn’t specify what project Riccio will lead. But recent speculation has focused on efforts by the company to develop a high-end virtual reality headset, or augmented reality glasses.

Apple is a holding in Jim Cramer’s Action Alerts PLUS member club. Want to be alerted before Jim Cramer buys or sells AAPL? Learn more now.



Read original article here

Astronomers Have Discovered a Star That Survived Being Swallowed by a Black Hole

When black holes swallow down massive amounts of matter from the space around them, they’re not exactly subtle about it. They belch out tremendous flares of X-rays, generated by the material heating to intense temperatures as it’s sucked towards the black hole, so bright we can detect them from Earth.

 

This is normal black hole behaviour. What isn’t normal is for those X-ray flares to spew forth with clockwork regularity, a puzzling behaviour reported in 2019 from a supermassive black hole at the centre of a galaxy 250 million light-years away. Every nine hours, boom – X-ray flare.

After careful study, astronomer Andrew King of the University of Leicester in the UK identified a potential cause – a dead star that’s endured its brush with a black hole, trapped on a nine-hour, elliptical orbit around it. Every close pass, or periastron, the black hole slurps up more of the star’s material.

“This white dwarf is locked into an elliptical orbit close to the black hole, orbiting every nine hours,” King explained back in April 2020.

“At its closest approach, about 15 times the radius of the black hole’s event horizon, gas is pulled off the star into an accretion disk around the black hole, releasing X-rays, which the two spacecraft are detecting.”

The black hole is the nucleus of a galaxy called GSN 069, and it’s pretty lightweight as far as supermassive black holes go – only 400,000 times the mass of the Sun. Even so, it’s active, surrounded by a hot disc of accretion material, feeding into and growing the black hole.

 

According to King’s model, this black hole was just hanging out, doing its active accretion thing, when a red giant star – the final evolutionary stages of a Sun-like star – happened to wander a little too close.

The black hole promptly divested the star of its outer layers, speeding its evolution into a white dwarf, the dead core that remains once the star has exhausted its nuclear fuel (white dwarfs shine with residual heat, not the fusion processes of living stars).

But rather than continuing on its journey, the white dwarf was captured in orbit around the black hole, and continued to feed into it.

Based on the magnitude of the X-ray flares, and our understanding of the flares that are produced by black hole mass transfer, and the star’s orbit, King was able to constrain the mass of the star, too. He calculated that the white dwarf is around 0.21 times the mass of the Sun.

While on the lighter end of the scale, that’s a pretty standard mass for a white dwarf. And if we assume the star is a white dwarf, we can also infer – based on our understanding of other white dwarfs and stellar evolution – that the star is rich in helium, having long ago run out of hydrogen.

“It’s remarkable to think that the orbit, mass and composition of a tiny star 250 million light years away could be inferred,” King said.

Based on these parameters, he also predicted that the star’s orbit wobbles slightly, like a spinning top losing speed. This wobble should repeat every two days or so, and we may even be able to detect it, if we observe the system for long enough.

 

This could be one mechanism whereby black holes grow more and more massive over time. But we’ll need to study more such systems to confirm it, and they may not be easy to detect.

For one, GSN 069’s black hole is lower mass, which means that the star can travel on a closer orbit. To survive a more massive black hole, a star would have to be on a much larger orbit, which means any periodicity in the feeding would be easier to miss. And if the star were to stray too close, the black hole would destroy it.

But the fact that one has been identified offers hope that it’s not the only such system out there.

“In astronomical terms, this event is only visible to our current telescopes for a short time – about 2,000 years, so unless we were extraordinarily lucky to have caught this one, there may be many more that we are missing elsewhere in the Universe,” King said.

As for the star’s future, well, if nothing else is to change, the star will stay right where it is, orbiting the black hole, and continuing to be slowly stripped for billions of years. This will cause it to grow in size and decrease in density – white dwarfs are only a little bigger than Earth – until it’s down to a planetary mass, maybe even eventually turning into a gas giant.

“It will try hard to get away, but there is no escape,” King said. “The black hole will eat it more and more slowly, but never stop.”

The research has been published in the Monthly Notices of the Royal Astronomical Society.

A version of this article was first published in April 2020.

 

Read original article here

Apollo CEO Leon Black to Step Down Following Review of Jeffrey Epstein Ties

Leon Black plans to step down as chief executive of Apollo Global Management Inc. after an independent review revealed larger-than-expected payments to disgraced financier Jeffrey Epstein that it nevertheless deemed justified.

The monthslong review by Dechert LLP found no evidence that Mr. Black was involved in the criminal activities of the late Epstein, who was indicted in 2019 on federal sex-trafficking charges involving underage girls, according to a copy of the law firm’s report that was viewed by The Wall Street Journal.

In its report, Dechert found the fees that the billionaire had paid Epstein were for legitimate advice on trust- and estate-tax planning that proved to be of significant value to Mr. Black and his family. Mr. Black paid Epstein a total of $148 million, plus a $10 million donation to his charity—far more than was previously known.

Mr. Black wrote in a letter to Apollo’s fund investors that he would cede the role of CEO to co-founder Marc Rowan on or before his 70th birthday on July 31 while retaining the role of chairman. In the letter, a copy of which was viewed by the Journal, Mr. Black detailed other governance changes he is recommending to the board, including the appointment of more independent directors and the elimination of Apollo’s dual-class share structure.

Mr. Black also pledged to donate $200 million of his family’s money to women’s initiatives.

Read original article here