Physics!!! The grand blueprint of how the universe operates. But let’s not sugarcoat it – it gets confusing, fast. Especially when you try to untangle the familiar realm of classical physics from the slippery, mind-bending, time-warping world of special relativity. And here’s the kicker: it’s not that the laws of physics change when things get extreme; it’s that out perception gets distorted. Einstein, sharp as ever, didn’t just hand us a new set of rules – he gave us a mathematical lens to see how things really work when they get, shall we say, cosmic<\/em>. <\/p>\n\n\n\n Classical physics is like your reliable friend\u2014predictable, grounded, always making sense. You know the rules: F=ma<\/em>, gravity pulls you down, and things move when a force acts upon them. Newtonian physics is the sturdy foundation of rocket trajectories, planetary motion, and bridges that don\u2019t collapse (well, most of the time). It\u2019s the stuff of everyday life, where everything seems in perfect order.<\/p>\n\n\n\n But then… then you approach the event horizon<\/a><\/strong> of a black hole, or start pushing the speed of light, and things start to get seriously weird. Time stretches, distances warp, and mass balloons like an over-inflated tire. Cue special relativity, right? Well, hold on a second. Einstein wasn\u2019t saying that the universe itself is warping in some mystical way\u2014he was saying that it\u2019s our perception<\/strong> that changes under these extreme conditions. And that\u2019s a subtle but crucial distinction.<\/p>\n\n\n\n Let\u2019s start with Einstein\u2019s most famous equation: E=mc2<\/sup><\/a>. The rockstar of physics. This beauty tells us that energy (E) is equal to mass (m) multiplied by the speed of light squared (c2<\/sup>). A tiny bit of mass can be converted into a whopping amount of energy. Now, in classical physics, we like to keep mass and energy in their own separate corners\u2014two distinct concepts. But Einstein, the clever devil, showed us they\u2019re interchangeable.<\/p>\n\n\n\n Now let\u2019s throw in some classical physics<\/strong> to spice things up. Remember, weight equals mass times gravity: w=mg. Rearrange that, and mass becomes m=w\/g\u200b. If we substitute that into Einstein\u2019s equation, we get:<\/p>\n\n\n\n E = (w\/g)c2<\/sup><\/p>\n\n\n\n And what does this tell us? As gravity increases<\/strong>, energy decreases<\/strong>. This is classical physics shaking hands with relativity. What you\u2019re seeing\u2014mass seemingly increasing as an object nears the speed of light\u2014isn\u2019t reality. It\u2019s perception<\/strong> getting all twisted. Einstein\u2019s math is like a cosmic decoder ring, translating those distortions back into classical terms. It’s like a universal conversion chart\u2014only with more math and fewer measuring cups.<\/p>\n\n\n\n Let\u2019s raise the stakes a bit. Enter the Einstein Field Equations<\/a><\/em><\/strong>, the heart of general relativity. These equations describe how matter and energy warp spacetime itself. A simplified form of these equations looks like this:<\/p>\n\n\n\n G\u03bc\u03bd<\/sub>\u200b+\u039bg\u03bc\u03bd<\/sup>\u200b=8\u03c0T\u03bc\u03bd<\/sub>\u200b<\/p>\n\n\n\n I know, that\u2019s a mouthful. But here\u2019s the deal: G\u03bcv<\/sub> represents how gravity curves spacetime, and T\u03bc\u03bd<\/sub>\u200b is the stress-energy tensor, which basically tells us how matter and energy are distributed in spacetime. The equation tells us how spacetime bends in the presence of mass and energy, and in return, how spacetime influences the movement of objects.<\/p>\n\n\n\n Now, back to classical physics<\/strong> for a second: remember Newton\u2019s law of gravitation? F=G(m1<\/sub>m2<\/sub>)\/r2<\/sup>\u200b\u200b, which gives the force of gravity between two masses. It works well enough here on Earth, but get near a black hole and Newton\u2019s law starts to break down like an old bridge in need of repair. The curvature of spacetime becomes so extreme that Newton\u2019s formula just can\u2019t keep up. That\u2019s where Einstein\u2019s equations<\/strong> step in\u2014like the cosmic clean-up crew.<\/p>\n\n\n\n Newton\u2019s law is like the training wheels of gravity\u2014works fine for the small stuff\u2014but Einstein gives us the whole picture. He didn\u2019t replace Newton; he just extended classical physics into the bigger reality<\/strong>.<\/p>\n\n\n\n Picture this: you\u2019ve got a cannon designed to fire a projectile 300 yards here on Earth. Classical physics at work. The energy required to launch that cannonball is fixed based on its mass, the force of the explosion, and Earth\u2019s gravity. But let\u2019s take that cannon on a field trip across the solar system<\/strong>.<\/p>\n\n\n\n First stop: the Moon<\/strong>. Gravity here is much weaker than on Earth, so when you fire the cannonball, it\u2019s going to soar much farther than 300 yards. Why? Because the energy<\/strong> required to push against the Moon\u2019s weaker gravitational pull is less. Same cannon, same energy, but gravity isn\u2019t doing much to hold the ball down, so it flies.<\/p>\n\n\n\n Next stop: Jupiter<\/strong>. Now things get interesting. Jupiter\u2019s gravity is brutal\u2014far stronger than Earth\u2019s. Fire the cannonball with the same amount of energy, and it\u2019ll barely crawl 10 yards before Jupiter\u2019s massive gravitational pull drags it down. But here\u2019s the key: to make that cannonball go the same 300 yards as it did on Earth, you\u2019d need a lot more energy<\/strong>. The stronger the gravitational field, the more energy you need to fight against it.<\/p>\n\n\n\n So, what\u2019s the takeaway? The cannonball\u2019s behavior isn\u2019t just about how far it goes, but about how gravity alters the energy requirements<\/strong>. On Earth, a certain amount of energy is enough to fire it 300 yards. On the Moon, you get more bang for your buck because gravity isn\u2019t holding it back. But on Jupiter, gravity demands a lot more energy just to move the ball a few feet.<\/p>\n\n\n\n This analogy isn\u2019t just about gravity pulling things down; it\u2019s about how gravity impacts the energy required<\/strong> to make things move. When gravity increases, the energy required to overcome it skyrockets. Same object, same physics, but different energy demands depending on where you are in the universe.<\/p>\n\n\n\n Let\u2019s go back to the trusty cannon and its journey through the cosmos. We\u2019ve already established that firing it on Earth, the Moon, or Jupiter results in vastly different outcomes because gravity changes how far the cannonball flies. But it\u2019s not just about how gravity affects motion\u2014it\u2019s about how energy requirements and mass interact under different gravitational forces.<\/strong><\/p>\n\n\n\n Now, here\u2019s where it gets interesting\u2014and potentially confusing. Let\u2019s take Einstein\u2019s famous equation E=mc2<\/sup>, but modify it slightly using classical physics. Remember that weight is the mass of an object times gravity: w=mg. Rearrange that, and you get mass as m=w\/g. Substituting this into Einstein\u2019s equation, we get:<\/strong><\/p>\n\n\n\n E=(w\/g)c2<\/sup><\/sub><\/p>\n\n\n\n According to the saying in science, “mass is constant no matter the gravitational force,” but is that really true? When you switch the formula around, w=mg, it tells us that as gravity increases, so does the weight. The more gravitational force, the heavier the object feels. But wait\u2014if weight increases with gravity, why shouldn\u2019t mass also change under gravitational force? Think about it: weight is just a product of mass and gravity, so if gravity pulls harder, why do we assume mass stays the same?<\/strong><\/p>\n\n\n\n Here\u2019s where things get confusing. We measure a person\u2019s weight on Earth because of Earth\u2019s gravitational pull. To find someone\u2019s mass, we divide their weight by Earth\u2019s gravity. But what if mass isn\u2019t as constant as we think? What if mass actually changes with gravitational forces, but we\u2019ve been missing this all along? After all, weight is essentially how mass manifests under gravity, and maybe we\u2019re just scratching the surface of what mass really does in extreme conditions.<\/strong><\/p>\n\n\n\n This also leads to a fascinating possibility: if mass decreases in stronger gravitational fields, like near a black hole, perhaps the energy required to accelerate objects would change too. Could this mean less energy is needed to push an object faster? We can\u2019t just change the formulas around without care, but these thought experiments start pulling on threads that traditional physics might be overlooking.<\/strong><\/p>\n\n\n\n This cannon analogy isn\u2019t just about how far something flies based on gravity\u2014it\u2019s about how gravity might alter mass itself, forcing us to rethink the relationship between weight, mass, energy, and the gravitational field. It\u2019s the ultimate puzzle: we see mass as constant, yet weight and gravity are inseparable. We can\u2019t have one without the other, but maybe our perception of mass is just as distorted as our perception of time near the speed of light.<\/strong><\/p>\n\n\n\n It\u2019s no wonder physics feels so mind-bending\u2014the more we think we know, the more we start to question what we\u2019ve always accepted.<\/strong><\/p>\n\n\n\n And this brings us to the next mind-bending thought: speed. In classic physics, we know that if you fire a gun from a car traveling at 150 mph, the bullet\u2019s speed is the car\u2019s speed plus the gun\u2019s muzzle velocity. Simple addition, right? So why, when we try to apply this to the speed of light, does it all go pear-shaped? Earth\u2019s speed through space is roughly 600,000 meters per second, and light travels at just under 300,000,000 m\/s. If you point a laser in the same direction Earth is moving, classical physics says the beam\u2019s speed should be 300,000,000+600,000300,000,000 + 600,000300,000,000+600,000 m\/s. But according to Einstein\u2019s special relativity, the speed of light remains constant\u2014no matter how fast the Earth, or any other object, is moving.<\/strong><\/p>\n\n\n\n Wait a minute\u2014why doesn\u2019t the laser move faster? Classic physics says it should. The issue here is perception again. Light, like that projectile from the Saturn cannon, doesn\u2019t behave the way you\u2019d expect at high velocities. It\u2019s not that light slows down or speeds up; it\u2019s that our perception of speed, time, and distance shifts the faster we move. When things start approaching the speed of light, they play by a new set of rules\u2014rules that are consistent with the old ones but appear distorted because we\u2019re looking through a different lens. The problem isn\u2019t with light; it\u2019s with how we\u2019re trying to see light.<\/strong><\/p>\n\n\n\n Now, imagine an object traveling faster than light. According to classical physics, you\u2019d just add the speeds and be done with it. But with relativity, something curious happens. Anything faster than light becomes effectively invisible\u2014why? Because light emitted from such an object would be moving slower than the object itself. You wouldn\u2019t be able to see it; the object would outpace its own light, and our perception would fail to grasp its existence. It\u2019s not that the object can\u2019t exist, it\u2019s just that we can\u2019t observe it with the same tools we\u2019re used to.<\/strong><\/p>\n\n\n\n Here\u2019s another thing to consider: we might perceive anything moving at or near the speed of light as light itself. Human perception, being limited by the speed at which our brains process visual information, may just see fast-moving objects as light because their speed distorts our senses. This suggests that the speed of light could also act as a perceptual limit for us. So, when objects approach light speed, they appear indistinguishable from light. It\u2019s not that faster-than-light travel is impossible, but our biology may not be equipped to see it, compounding the mystery of what\u2019s truly happening at such speeds.<\/strong><\/p>\n\n\n\n And that\u2019s not all. When you bring in gravitational fields and the compression of matter, things get even more interesting. As atoms get squeezed under greater and greater gravitational fields, they slow down. Think of it like water freezing\u2014when water cools, the movement of its molecules slows down, though never completely stops. But what if, under the intense gravitational pull of a black hole, atoms constrict so much that they do<\/em> reach a point of zero movement\u2014absolute zero? This is the temperature at which atomic motion ceases, and while many scientists speculate that absolute zero is impossible to achieve, perhaps within a black hole\u2019s crushing gravitational force, it\u2019s not just a theory. It could be reality.<\/strong><\/p>\n\n\n\n This isn\u2019t just perception anymore\u2014this is classic physics at work. The nuclear forces that bind atoms and the electromagnetic forces that attract them are all players in the game, constricting under the weight of extreme gravity. Whether we\u2019re talking about zero gravity or infinite gravity, the principles stay the same. As gravity increases, so does the energy required to move within that gravitational field. This is where perception takes a backseat to what\u2019s really happening. Sure, we observe an increase in energy, but that energy is only equal to the amount of force being used to push an object through space.<\/strong><\/p>\n\n\n\n Take a star approaching a black hole. We often talk about the star \u201cfalling\u201d into the black hole, but in reality, it\u2019s being pulled by an immense gravitational force\u2014into what? Not a \u201chole\u201d at all, but a massive gravitational sphere, what you might call a super black star. Its gravity is so intense that not even light has enough energy to escape it. The forces at play here, from nuclear binding to electromagnetic attraction, are all working together, constricting under the enormous pressure of gravitational fields. What we observe is almost irrelevant to what\u2019s really happening unless we want to convert that observation into classical terms. Now let\u2019s get a bit more imaginative\u2014take the exact same cannon that fires a projectile 300 yards here on Earth and bring it to Saturn. If you could stand on Saturn (we\u2019ll assume for this experiment that you won\u2019t be crushed by its immense gravity), you\u2019d find the cannonball barely makes it 10 yards. Saturn\u2019s gravity is so strong that it consumes the energy, pulling the projectile down faster than it would here on Earth. Yet, an observer from a distance might see that cannonball soaring forever because their perception is distorted by the gravitational field.<\/strong><\/p>\n\n\n\n Let\u2019s move from light-speed to biological decay and time itself. Time, we say, is just a construct\u2014our way of making sense of events. Take the atomic clock\u2014this precise timekeeper uses the decay of specific atoms to measure time with mind-boggling accuracy.<\/strong><\/p>\n\n\n\n But throw gravity into the mix, and things get messy. The stronger the gravity, the slower those atoms decay. Near a black hole, atomic decay would slow down so much you\u2019d practically need eternity to finish a game of chess. This is more than just perception\u2014this is classic physics in action. The same goes for biological decay. Gravity\u2019s time-stretching effects would make living things age more slowly in intense gravitational fields. Get too far from gravity, and things might decay faster\u2014who knows, we could even age out of existence. Gravity, in a sense, is like the universal clockmaker<\/strong>, ticking faster or slower depending on how close you get to its gravitational pull. Time isn\u2019t fixed\u2014it stretches and contracts based on the forces at play.<\/strong><\/p>\n\n\n\n Here\u2019s another curveball: faster-than-light travel. Classical physics, says that as you approach the speed of light, energy demands go through the roof, theoretically becoming infinite because its mass increases with speed. But when we replace mass with w\/g (weight divided by gravity), we are introducing an idea where gravitational fields could reduce effective mass. And right\u2014if gravitational forces are factored in, as they increase, the effects on mass change. This means that the energy demands could<\/em> decrease under the right circumstances. Classical physics would indeed suggest that as mass decreases (or approaches zero), energy lessens. This hints that, under extreme gravitational fields, like those near black holes, under extreme gravitational conditions, faster-than-light travel isn\u2019t so impossible after all.<\/strong><\/p>\n\n\n\n Now, in a strong gravitational field (like near a black hole), objects experience significant “spacetime warping.” If mass decreases as gravity increases (which aligns with some speculative ideas in general relativity and quantum theory), the energy needed to accelerate could, in theory, decrease, potentially bypassing the known limits of light speed. I propose that it\u2019s not impossible, but just incredibly difficult based on our current understanding and technological limits.<\/strong><\/p>\n\n\n\n Take a star approaching a black hole<\/a>. We often talk about the star \u201cfalling\u201d into the black hole, but in reality, it\u2019s being pulled by an immense gravitational force\u2014into what? Not a \u201chole\u201d at all, but a massive gravitational sphere, what you might call a super black star (I theorize a black star is a massive star that has not become a black hole. It has just enough gravitational force to keep light from escaping but not an event horizon). Its gravity is so intense that not even light has enough energy to escape it. The forces at play here, from nuclear binding to electromagnetic attraction, are all working together, constricting under the enormous pressure of gravitational fields. What we observe is almost irrelevant to what\u2019s really happening unless we want to convert that observation into classical terms.<\/strong><\/p>\n\n\n\n Now, let\u2019s get even cosmologically wilder: what if we could harness the colossal energy near a black hole (which we\u2019re still far from achieving), is it conceivable that we could manipulate spacetime itself? Einstein\u2019s equations don\u2019t explicitly forbid faster-than-light travel\u2014they just set tough conditions, like needing for exotic forms of energy or matter (like negative energy or antimatter) to create something like a “warp bubble.” What if using black hole energy to manipulate an object’s mass and energy requirements plays on a similar concept? Black hole energy could theoretically reduce an object\u2019s mass or warp spacetime in ways that allow it to skirt the speed-of-light barrier; past the light barrier – some kind of comic catchphrase. This isn\u2019t too far from ideas like the Alcubierre drive<\/a>\u2014a hypothetical concept \u2013 which proposes moving faster than light by warping spacetime itself. Black holes could be nature\u2019s shortcut through the cosmic speed limit, bending spacetime just enough to get us where we want to go \u2013 faster than light but without breaking any major universal laws.<\/strong><\/p>\n\n\n\n Speaking of breaking the rules, ever heard of virtual particles? In quantum field these little guys pop in and out of existence so fast it makes your head spin. It\u2019s like they\u2019re borrowing energy from the universe and then ducking out before anyone notices. What if these particles are actually moving faster than light, zipping through a reality we just cannot perceive. <\/strong><\/p>\n\n\n\n The idea isn\u2019t so far-fetched. If something outruns its own light, it would appear to blink in and out of existence \u2013 seeming to break the rules, when really, it\u2019s just playing by a set of rules we haven\u2019t fully grasped yet. Welcome to quantum weirdness of it all.<\/strong><\/p>\n\n\n\n Einstein wasn\u2019t giving us new laws; he was giving us a new way to see the laws we already knew. The math of special relativity is the tool to translate what happens at these extreme ends of physics back into something we can grasp with our classical understanding. It\u2019s not about changing reality\u2014it\u2019s about adjusting our perception of reality, especially when conditions push us beyond our usual frame of reference.<\/strong><\/p>\n\n\n\n Whether atoms slow down and constrict under the crushing weight of a black hole or objects get pulled into the swirling gravitational field of a black star(hypothetical star that has not turned into a black hole and does not have an event horizon), the truth stays the same: classical physics governs the fundamental forces, and relativity helps us decode how our perceptions get warped in extreme environments.<\/strong><\/p>\n\n\n\n For a hundred years, people have treated special relativity like it\u2019s some sort of revolutionary, alien science. But really, it\u2019s a philosophical shift. It\u2019s a framework that helps us reconcile what we see with what\u2019s true. And that truth is grounded in classical physics: objects still follow the same rules, energy is conserved, and mass isn\u2019t mysteriously growing\u2014it\u2019s just how we perceive those things that shifts when gravitational fields or speeds near light take over.<\/strong><\/p>\n\n\n\n Einstein didn\u2019t hand us a whole new rule-book \u2013 he gave us the tools to reconcile what we see with what\u2019s really happening. And when it comes down to it, seeing isn\u2019t always being. That\u2019s the genius of Einstein. And you know what? After a century of confusion, it\u2019s about time we start getting it right.<\/strong><\/p>\n","protected":false},"excerpt":{"rendered":" Physics: it’s where your brain gives up trying to understand if cats are alive or dead in boxes. Classical physics is your dependable pal, but throw in Einstein\u2019s relativity, and things get wacky. Light speed doesn\u2019t mix with Newton\u2019s equations; it\u2019s like adding pineapple to pizza \u2013 controversial! Einstein didn\u2019t rewrite rules, he handed us the ultimate cosmic decoder ring to decode reality\u2019s quirks. Gravity, perception, and zipping faster (or not) than light, it\u2019s the science equivalent of a mind-bending rollercoaster \u2013 guaranteed fun, confusion, and a headache!<\/p>\n","protected":false},"author":1,"featured_media":146,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_jetpack_memberships_contains_paid_content":false,"footnotes":""},"categories":[21],"tags":[],"class_list":["post-142","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-science"],"featured_image_urls":{"full":["https:\/\/itsscientificjack.com\/wp-content\/uploads\/2024\/10\/PhysicsArticleConfusing-e1727989958794.jpg",350,350,false],"thumbnail":["https:\/\/itsscientificjack.com\/wp-content\/uploads\/2024\/10\/PhysicsArticleConfusing-150x150.jpg",150,150,true],"medium":["https:\/\/itsscientificjack.com\/wp-content\/uploads\/2024\/10\/PhysicsArticleConfusing-300x300.jpg",300,300,true],"medium_large":["https:\/\/itsscientificjack.com\/wp-content\/uploads\/2024\/10\/PhysicsArticleConfusing-e1727989958794.jpg",350,350,false],"large":["https:\/\/itsscientificjack.com\/wp-content\/uploads\/2024\/10\/PhysicsArticleConfusing-e1727989958794.jpg",350,350,false],"1536x1536":["https:\/\/itsscientificjack.com\/wp-content\/uploads\/2024\/10\/PhysicsArticleConfusing-e1727989958794.jpg",350,350,false],"2048x2048":["https:\/\/itsscientificjack.com\/wp-content\/uploads\/2024\/10\/PhysicsArticleConfusing-e1727989958794.jpg",350,350,false],"trp-custom-language-flag":["https:\/\/itsscientificjack.com\/wp-content\/uploads\/2024\/10\/PhysicsArticleConfusing-12x12.jpg",12,12,true],"newsphere-slider-full":["https:\/\/itsscientificjack.com\/wp-content\/uploads\/2024\/10\/PhysicsArticleConfusing-e1727989958794.jpg",350,350,false],"newsphere-featured":["https:\/\/itsscientificjack.com\/wp-content\/uploads\/2024\/10\/PhysicsArticleConfusing-e1727989958794.jpg",350,350,false],"newsphere-medium":["https:\/\/itsscientificjack.com\/wp-content\/uploads\/2024\/10\/PhysicsArticleConfusing-512x380.jpg",512,380,true],"mailpoet_newsletter_max":["https:\/\/itsscientificjack.com\/wp-content\/uploads\/2024\/10\/PhysicsArticleConfusing-e1727989958794.jpg",350,350,false],"woocommerce_thumbnail":["https:\/\/itsscientificjack.com\/wp-content\/uploads\/2024\/10\/PhysicsArticleConfusing-300x300.jpg",300,300,true],"woocommerce_single":["https:\/\/itsscientificjack.com\/wp-content\/uploads\/2024\/10\/PhysicsArticleConfusing-e1727989958794.jpg",350,350,false],"woocommerce_gallery_thumbnail":["https:\/\/itsscientificjack.com\/wp-content\/uploads\/2024\/10\/PhysicsArticleConfusing-100x100.jpg",100,100,true]},"author_info":{"display_name":"scientificjack","author_link":"https:\/\/itsscientificjack.com\/author\/scientificjack"},"category_info":"Science<\/a>","tag_info":"Science","comment_count":"0","jetpack_featured_media_url":"https:\/\/itsscientificjack.com\/wp-content\/uploads\/2024\/10\/PhysicsArticleConfusing-e1727989958794.jpg","jetpack_sharing_enabled":true,"jetpack_likes_enabled":true,"brizy_media":[],"_links":{"self":[{"href":"https:\/\/itsscientificjack.com\/index.php?rest_route=\/wp\/v2\/posts\/142","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/itsscientificjack.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/itsscientificjack.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/itsscientificjack.com\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/itsscientificjack.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=142"}],"version-history":[{"count":4,"href":"https:\/\/itsscientificjack.com\/index.php?rest_route=\/wp\/v2\/posts\/142\/revisions"}],"predecessor-version":[{"id":151,"href":"https:\/\/itsscientificjack.com\/index.php?rest_route=\/wp\/v2\/posts\/142\/revisions\/151"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/itsscientificjack.com\/index.php?rest_route=\/wp\/v2\/media\/146"}],"wp:attachment":[{"href":"https:\/\/itsscientificjack.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=142"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/itsscientificjack.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=142"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/itsscientificjack.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=142"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}First Example: E = mc2<\/sup><\/h2>\n\n\n\n
Second Example: Einstein’s Field Equations<\/h2>\n\n\n\n
The Cannon and Energy: A Gravity Lesson<\/h2>\n\n\n\n
The Cannon, Energy, and the Gravitational Puzzle<\/h2>\n\n\n\n
Speed and Perception: A Relativity Paradox<\/strong><\/h2>\n\n\n\n
Atomic Clocks, Biological Decay, and Gravity\u2019s Impact<\/strong><\/h2>\n\n\n\n
Faster-than-Light Travel and Energy<\/h2>\n\n\n\n
Harnessing the Energy of a Black Hole<\/strong><\/h2>\n\n\n\n
Particles Popping In and Out of Existence<\/strong><\/h2>\n\n\n\n
Final Thoughts: Perception and Reality<\/strong><\/h2>\n\n\n\n