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    Black Hole Theory Cosmology (WHAT ARE BLACK HOLES?!) Part 2 with Ronald Gamble, Jr.

    en-usFebruary 28, 2024

    Podcast Summary

    • Accurate depiction of black hole visuals in InterstellarTheoretical astrophysicist confirms Interstellar's portrayal of a black hole's light bending effect and time dilation is accurate

      The movie "Interstellar" does a commendable job depicting the visual aspects of a black hole, according to theoretical astrophysicist and black hole theory cosmologist, doctor Ronald Gamble. He confirmed that the scene of light curving around the black hole, known as Gargantua in the movie, is an accurate representation of what one might see if they were to get extremely close to a super massive black hole. The movie's portrayal of time dilation, where time passes much slower for objects near a black hole, was also confirmed to be accurate by Gamble, who mentioned that the film had a good consultant in the form of Kip Thorne, a Nobel Prize winner in physics.

    • Understanding Black Holes: Mass, Spin, Event Horizon, and BrightnessBlack holes are massive cosmic entities defined by their mass, spin, event horizon, and brightness or entropy. Supermassive black holes, located at the center of galaxies, differ in scale but share similar properties.

      Black holes, despite their ominous reputation, can be understood through simple concepts such as mass, spin, event horizon, and brightness or entropy. The term "stupendously large black holes" has emerged as an official science term for those with a mass greater than 100 billion times that of our Sun. Visual effects teams in movies like Interstellar have contributed to scientific understanding by simulating black hole imagery and publishing findings. Supermassive black holes, located at the center of galaxies, differ only in scale from regular black holes. Scientists study these properties to observe and understand black holes, which emit light from the matter surrounding them.

    • Black holes emit phenomena like jets and have a lifespanBlack holes don't just swallow matter, they also emit jets and have a lifespan, with smaller ones evaporating over time

      Black holes are not just empty voids in space. They emit various phenomena, such as relativistic jets, which can be thought of as "black hole lighthouses" or "black hole lasers." These emissions are not coming from inside the black hole but rather from its surroundings. Black holes also have a lifespan, although the exact method to calculate it is not yet known. The theory of evaporating black holes suggests that they lose mass and energy over time due to the creation and escape of particle-antiparticle pairs, leading to their eventual disappearance. This process, however, is a gradual one and applies mainly to smaller black holes. The larger ones, like the supermassive black hole at the center of the Milky Way, are believed to be long-lived due to their immense size.

    • The vastness of time and space challenges our understanding of the universeFrom gravitational pair production and black hole evaporation to observing the Big Bang and potential wormholes, the universe continues to reveal new complexities, leaving many questions unanswered.

      Our understanding of the universe continues to expand, challenging our current theories and revealing new possibilities. For instance, the idea that everything with gravity, including ourselves, will eventually evaporate due to a process called gravitational pair production and black hole evaporation, is a humbling reminder of the vastness of time. Furthermore, as we look deeper into space, we're essentially peering further back in time, which can be mind-boggling when considering the time it takes for light to reach us. The possibility of observing a black hole evaporate is an exciting prospect, although it remains a scientific goal. The relationship between the Big Bang and black holes is complex and requires an understanding of advanced theories like string theory and M theory, which propose the existence of multiple universes. One intriguing concept is the idea that black holes and white holes, their symmetric counterparts, could be connected, creating a "tube" called a wormhole. This theoretical construct could potentially allow for travel through space and time, adding another layer to our understanding of the cosmos. However, despite these fascinating ideas, many questions remain unanswered, such as the nature of white holes and their potential detectability. The ongoing exploration of these concepts will undoubtedly lead to new discoveries and a deeper appreciation for the wonders of the universe.

    • Exploring the mysteries of wormholesWormholes, theoretical shortcuts through space-time, could potentially allow for faster-than-light travel and are studied for their potential to unlock new possibilities for space travel and understanding the universe, despite their complex and mind-bending nature.

      Wormholes, theoretical shortcuts through space-time, remain an intriguing and complex topic in physics research. They are hypothesized to be formed by folding and connecting two sheets of space-time, requiring exotic matter or quantum entanglement to keep them open. Wormholes could potentially allow for faster-than-light travel across vast distances, but the nature of the bridge connecting the two sheets of space-time remains a mystery. The idea of traversing wormholes can evoke feelings of anxiety and vertigo due to their mind-bending properties, but scientists continue to explore this fascinating concept, hoping to unlock new possibilities for space travel and understanding the universe.

    • Exploring the Unknown: Black Holes and the Reality of UncertaintyBlack holes have implications in our everyday lives, but conspiracy theories about the Large Hadron Collider creating black holes or portals are unfounded. Science is a continuous process of discovery and learning, embracing uncertainty and probability.

      While we are curious and anxious about discovering new phenomena like black holes, we also face the reality that we may not have all the answers yet. This uncertainty can lead to panic, but ultimately, we push forward and continue to explore and learn. Black holes, despite their mysterious nature, have implications in our everyday lives through technologies like GPS and 5G. Contrary to conspiracy theories, the Large Hadron Collider does not create black holes or portals to other universes. Instead, it operates within the known laws of physics. Quantum mechanics, which underpins our understanding of the subatomic world, is based on probability and uncertainty. It's important to remember that science is a process of continuous discovery and learning, and it's okay not to have all the answers yet.

    • Every decision creates a new universe or timelineQuantum mechanics introduces the concept of infinite possibilities and alternate realities, challenging our understanding of reality and existence, and reminding us to appreciate the present moment.

      According to quantum mechanics, every decision or event creates a new universe or timeline, leading to an infinite number of possibilities and versions of ourselves and the world around us. This concept, known as multiverses or branching timelines, challenges our understanding of reality and existence. It raises questions about the nature of causality and the interconnectedness of events. It also highlights the anxiety of considering the potential consequences of our choices and the existence of alternate realities where things are different. Despite the complexities, it serves as a reminder to appreciate and maximize the present moment, as we only have one reality that we can experience and influence.

    • Indirect Evidence of Black Holes: Gravitational Lensing, Einstein Crosses, and Hawking RadiationBlack holes cannot be directly seen but their presence is inferred through phenomena like gravitational lensing, Einstein crosses, and the belief that they emit Hawking radiation

      While we can observe the effects of black holes on other objects through phenomena like gravitational lensing and Einstein crosses, we cannot directly see black holes themselves due to their inherent darkness. Instead, we rely on indirect evidence such as the behavior of nearby matter and radiation like Hawking radiation to infer their presence. For instance, the closest known black hole, Gaia bhone, is about 1500 light years away, which is still millions of miles away from us, and we cannot travel to it. Hawking radiation is a form of quantum thermal fluctuations, or heat, that is believed to be emitted by black holes on a subatomic scale. Although we have not yet observed Hawking radiation directly, we have attempted to detect it and hope to do so in the future with advanced technology. Despite our limited ability to directly observe black holes, their profound impact on the universe continues to fascinate and challenge scientists.

    • The Mystery of Information in Black HolesBlack holes cause a decrease in total information as anything thrown in is lost forever, leaving the universe beyond the event horizon a mystery

      The information paradox is a concept in physics that raises questions about what happens to information when it enters a black hole. If we consider a Rubik's cube as an example of information, when it's thrown into a black hole, it's lost to our universe, leading to a decrease in total information. This is known as an irreversible process, as once something enters a black hole, we cannot get it back. The universe beyond the event horizon is a mystery, and theories suggest that if all matter were to be tossed into a black hole, the universe might not exist anymore. Black Hole Sun by Soundgarden is a song that references this concept, with the lyrics expressing a desire for the black hole to wash away troubles, but the meaning behind it is open to interpretation. The information paradox remains an intriguing and complex topic in theoretical physics.

    • Detection of Gravitational Waves from Black Hole MergerFirst direct evidence of black hole merger detected by LIGO, releasing massive energy in the form of gravitational waves, confirming Einstein's theory of general relativity.

      During a black hole merger, a massive amount of energy is released in the form of gravitational waves. This was first detected by LIGO, the Laser Interferometer Gravitational Wave Observatory, in 2019. The merging black holes, each with significant mass, create a violent process that results in the smearing of their event horizons. This event confirms a key prediction of Einstein's theory of general relativity and provides the first direct evidence that black holes merge. The sound of this event, when sonified, produces a chirp or a whoop-like sound. The discussion also revealed that Muse's song "Supermassive Black Hole" is about the band's fascination with black holes and the power of women, with the vocalist, Matthew Bellamy, considering women as his muse.

    • Detection of Gravitational Waves and Their SignificanceIn 2015, LIGO detected gravitational waves, confirming Einstein's theory of relativity and marking a major milestone in astronomy. These waves, caused by massive objects accelerating, are ripples in space-time. Black holes are smaller than expected, and getting 'spaghettified' in a gravitational field is a slow process with no pain.

      Gravitational waves are ripples in space-time caused by massive objects accelerating through the universe. These waves were detected for the first time in 2015 by the Laser Interferometer Gravitational-Wave Observatory (LIGO) using highly sensitive interferometers that can measure tiny displacements on the scale of 10 to the power of -20 meters. This detection confirmed a major prediction of Albert Einstein's general theory of relativity and marked a significant milestone in the field of gravitational wave astronomy. Additionally, getting "spaghettified" in a gravitational field would not be painful as one would not feel it due to the extremely slow process involved. The size of a black hole, when measured by its event horizon, is smaller than one might expect, possibly on the scale of the Earth's radius. These discoveries represent a major step forward in our understanding of the universe and the fundamental forces that govern it.

    • The Universe's Vastness and Enormous StructuresThe universe is filled with immense structures, like the super massive black hole TON 618, which challenges our perspective and understanding.

      The universe contains incredibly large structures, such as the super massive black hole TON 618, which has an event horizon larger than our solar system. This black hole, which is about 100 times the mass of the center of our galaxy, puts our Milky Way into perspective as a small bird on its head. The vastness of the universe and the existence of such enormous structures can be both awe-inspiring and anxiety-inducing. Discoveries in physics often come from imagination and thought experiments, which can lead to new equations and understanding of the physical world. However, explaining new theories to both old theorists and the general public can be a challenge. Despite the unknowns and the difficulty of understanding the universe's complexities, the pursuit of knowledge and discovery keeps scientists working late into the night.

    • The value of embracing the unknown through questioning and correspondence in scienceContinuously asking questions and engaging in correspondence with others can lead to new scientific discoveries and advancements in understanding

      The pursuit of knowledge is a continuous process, and not knowing everything is a natural part of it. During a talk at St. Andrew's Episcopal High School in Delaware, students asked thought-provoking questions that challenged the speaker's knowledge. This experience highlighted the importance of embracing the unknown and the value of asking questions. The history of science is filled with examples of scientists challenging each other's theories through lengthy, private letters. One such instance involved physicists Dayton Miller and Robert Shanklin's correspondence regarding Einstein's theory of relativity. Despite their disagreements, the exchange of ideas led to advancements in scientific understanding. The mystery of black holes is another example of the allure of the unknown in science. While we have made progress in understanding these phenomena, there is still much to discover. The best thing about black holes, as the speaker noted, is the mystery they present and the continuous drive to learn more.

    • Exploring the Universe's Secrets: A Long and Rewarding JourneyContinuously learn new math, think creatively, ask brilliant questions, keep detailed notes, and stay curious to unravel the universe's mysteries, potentially enhancing your romantic life.

      Understanding the mysteries of the universe, including black holes, requires a deep understanding of complex mathematical concepts and continuous creativity. The speaker, a scientist, emphasizes the importance of learning new math and thinking outside the box to make new connections and discoveries. She also encourages asking brilliant people questions and keeping detailed notes for future reference. The journey to unraveling the secrets of the universe may be long and challenging, but the rewards are immense. So, keep learning, stay curious, and remember that every piece of information, no matter how small, could be a key to unlocking a greater understanding. And who knows, your romantic life might even blossom along the way!

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    Cosmology (THE UNIVERSE) Part 1 Encore with Katie Mack

    Cosmology (THE UNIVERSE) Part 1 Encore with Katie Mack

    Stars. Black holes. THE GAWDANG UNIVERSE. Astrophysicist and cosmologist Dr. Katie Mack (@astrokatie) re-introduces us to this 2017 episode along with some bonus updates on astrophysics, her career, and the book she’s published since we last heard from her. Katie also tells us her most embarrassing moments as a cosmologist, debunks some physicist myths and gives us the nuts + bolts of everything form particle physics to gravitational waves and existential mysteries. Walk away with cocktail party comprehension of everything from the itty-bitty quarks that make you to the neutron stars banging together across the cosmos. More than anything, get perspective about your life on this, our little pale blue dot.

    Visit Dr. Mack’s website and follow her on Instagram, Twitter, YouTube and TikTok

    Buy Dr. Mack's new book: The End of Everything (Astrophysically Speaking)

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    Editing by Steven Ray Morris and Mercedes Maitland of Maitland Audio Productions

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    002 - Lawrence Krauss Ph.D

    002 - Lawrence Krauss Ph.D

    In this episode, Robert talks with Lawrence M. Krauss, Ph.D., world-renowned theoretical physicist, acclaimed lecturer, and bestselling author. 

    They discuss their views and experiences related to Quantum Mechanics, Quantum Cryptography, Quantum Entanglement, Faster-than-light Communication, Free Speech, Echo Chambers, and many other interesting subjects.

    Prof. Krauss is the author of over 500 publications and numerous popular articles on physics and astronomy. Among Lawrence's numerous scientific contributions was the proposal, in 1995, that most of the energy of the Universe resided in empty space. This prediction was verified in 1999 by two teams of astronomers, and the discovery was awarded the Nobel Prize in 2011.

    It's wonderful to have two great minds bringing important considerations that challenge the world's current predominant paradigms to the surface. We hope you enjoy their spirited debate and can extract valuable insights from the different perspectives shared in this remarkable encounter!

    If you haven't already done so, subscribe to my channel, leave a comment, and share this episode with your friends.

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    Episode 5 - Thunder Lightening & Black Holes

    Episode 5 - Thunder Lightening & Black Holes
    Lightening, ... Thunder, Lightening, ... Thunder. August in Ontario is awesome for natural displays of destruction and beauty. Everyone knows that light and sound travel at very different speeds, so when you see a flash of lightening, you can count until you hear the thunder to see how far away the lightening occurred. Roughly 3 seconds for every KM. But how does a flash of light create a deafening boom?  It all has to do with plasma. Plasma occurs when you have a high energy reaction that strips electrons off the raw nuclei of their atoms. This results in a state of matter so unstable it creates ionizing radiation, like ultra violet, x-rays and gamma radiation, it's highly susceptible to the effects of electromagnetic fields, and get's extremely hot, very fast.
     
    When you have a large charge differential between clouds in the atmosphere or the clouds and ground, you can create an arc. Basically the air breaks down along these long filaments and the gas itself becomes conductive. All the electrons caught in this eddy of electromagnetism zip off of their orbitals and rush to the positive side of the charge. This causes a sudden flash of plasma. Remember electrons popping up and down between excited states causes excitation in the electromagnetic field. The larger the orbital jump, the higher energy the photon produced. There's your flash. It sweeps across the whole EM field, You're able to see it, smell it, and pick it up on radios on the other side of the planet. All of those electrons being torn away from their comfy atoms all at once means you suddenly have a massive positive charge in the atmosphere. So you get a "Coulomb Explosion". The air effectively detonates, flying apart as the nuclei are no longer held in check by their electrons. The charges are imbalanced and the air explodes creating thunder.
     
    I know this is a stretch, but a similar process can be found in the heart of dying stars. Every bolt of lightening, we experience here is like a miniature super-nova. Seems like the world we live in currently is a kin to stellar destruction. Let's look at the last moments of a large star before it goes super-nova. 
     
    For millions or sometimes, billions of years, a star spends its life fusing hydrogen into helium. It then starts to fuse elements that are a bit heavier, leading up iron. Once iron comes into the equation, things get very bad very quickly. Suddenly, it’s no longer able to sustain equilibrium, because iron takes so much energy to produce, the reaction of fusion turns from exothermic to endothermic, the core collapses in on itself, all it's outer fusion layers are in free-fall until they crash against the much smaller core and rebound in a coulomb shockwave, casting off the plasma envelope and sparking a supernova. 
     
    The only thing that keeps a star in check is the delicate balance between the energy being created on the inside, and the mass, or gravity, of the star that holds it together. When the shockwave propagates through the star, it pushes a lot of the material away at a speed much greater than the escape velocity of the Iron core. Since all the fusion and energy created insanely hot plasma, the star can no longer hold its form and completely breaks down. The exposed nuclei of the stellar plasma repels against itself as it is unable to keep its electrons at that high energy. The star explodes. Cosmic thunder.
     
    What happens next is completely a product of mass and density. You get either a Neutron star a pulsar or a black hole. Now a black hole is a curious thing. The main distinction here is the event horizon. Turns out everything has an event horizon. It's a sphere where if you were to compress all the mass of an object down to a certain point, you can create a black hole. If you took Mount Everest and tried to fit it into its own event horizon, it would be smaller than a proton. However, if you tried to cram the entire Earth into its own event horizon, you would have an object the size of a peanut. The sun would be only around 3 KM if you crammed it into its event horizon. 
     
    People don't really know what happens when a black hole is created. What happens beyond that event horizon. It's called an EVENT horizon, because everything that falls into it, is Causally disconnected from the rest of the universe from that point forward. It's a tipping point where space itself is rushing toward the center of the gravity well faster than the speed of light. Making any outward flow if information completely impossible. This acceleration also means that anything falling into the black hole experiences massive time dilation. 
     
    Essentially, anyone watching you fall into a black hole would never see you cross the event horizon. You would approach the blackness, then start to move very slowly, the light coming off you would shift red, then to microwaves, then radio waves, then be completely imperceptible, as your image blurs and fades into nothingness on the surface of the event horizon. The time dilation approaches infinity beyond the event horizon, so there you are, frozen in time... to the outside observer. 
     
    But from your point of view, you would just keep falling in. The whole universe would start changing, shifting blue, as you cross rubicon. Eventually, you would be torn apart by the inrush of high energy radiation, as the clockworks of the entire universe play out in a fast-forward ballet. All of this happens long before you experience Spaghetification, and tidal forces stretch your atoms into a thin stream of matter destined for the singularity.
     
    I had an interesting thought when researching this. What if the same rebound forces that occur within supernovae are present in black holes? The star collapses as usual, and rebounds as usual into a super nova, but the fact that the star collapsed into its own event horizon, means the time dilation for the rebound blast wave completely obscures the resulting supernova. Time is stopped. Frozen just before impact. Hovering, like held breath, like the anticipation before your first teenage kiss. A logarithmic curve that will approach zero forever.
     
    When will the black holes release their secrets, and we are once again reunited with everything we've lost to time. It may be when we master, and transcend our causal connections. Casting off our temporal shackles and exist in the forever now. Until then, take a deep breath, close your eyes, and wait for your logarithmic kiss. Forever just hovering a moment away.

    Diving Into Black Holes

    Diving Into Black Holes
    In this episode of Big Ideas Only, we discuss the topic of black holes, white holes, and wormholes: What are they and why are they so interesting to look at.

    Today, our guest is Ole Eggers Bjælde, an astrophysicist at Aarhus University. He’ll explain what black holes are, how they work, and what would happen if you get sucked into one.

    Your host is Mikkel Svold, CEO of Montanus.

    This podcast is produced by Montanus, https://montanus.co