What is *Antimatter* by Frank Close about?

*Antimatter* explores the mysterious counterpart to ordinary matter, tracing its discovery from Paul Dirac’s groundbreaking equation to modern particle physics research. Frank Close explains antimatter’s properties, its role in the universe’s origins, and addresses myths about its applications in energy and weapons. The book blends scientific history, cosmic mysteries, and real-world uses like medical imaging, offering an accessible dive into subatomic physics.

Who should read *Antimatter* by Frank Close?

Science enthusiasts, physics students, and general readers curious about particle physics will find this book engaging. Close’s clear explanations make complex concepts like annihilation, cosmic rays, and antimatter production approachable for non-experts. It’s ideal for those interested in debunking sci-fi myths or understanding why the universe favors matter over antimatter.

Is *Antimatter* by Frank Close worth reading?

Yes—the book is praised for distilling complex physics into digestible insights without oversimplifying. Close balances historical context (e.g., the Tunguska event speculation) with modern research, while clarifying misconceptions about antimatter bombs and energy. Some readers note challenging sections on mathematical matrices, but overall, it’s a compelling primer on one of physics’ most enigmatic topics.

What is the Dirac equation, and why is it important in *Antimatter*?

Paul Dirac’s 1928 equation predicted antimatter’s existence by reconciling quantum mechanics and relativity. Close highlights its elegance, showing how it revealed particles’ “mirror” counterparts and revolutionized physics. The equation remains foundational for understanding antimatter production in particle accelerators and the universe’s matter-antimatter asymmetry.

How does *Antimatter* address science fiction myths?

Close debunks popular myths, like antimatter as a limitless energy source or clean weapon, clarifying that production costs exceed energy output and annihilation releases harmful gamma rays. He contrasts these with real applications: PET scans and theoretical spacecraft propulsion. This myth-vs-reality framework helps readers separate Hollywood fantasies from scientific feasibility.

What caused the universe’s matter-antimatter imbalance?

A central mystery explored in the book, the imbalance suggests antimatter largely disappeared after the Big Bang. Close discusses theories like CP violation (differences in matter-antimatter behavior) and ongoing experiments at CERN to explain why matter dominates—a question pivotal to understanding cosmic evolution.

Does *Antimatter* discuss real-world applications?

Yes. While dismissing fictional uses, Close details antimatter’s role in PET scans, which image bodily processes using positrons. He also explores speculative ideas like antimatter-powered spacecraft, though notes technical hurdles like storage. These examples highlight its value in medicine and fundamental physics research.

What historical events are linked to antimatter in the book?

Close examines the 1908 Tunguska explosion, once theorized as an antimatter meteor impact—a hypothesis later disproven. He also covers key scientific milestones: Carl Anderson’s 1932 discovery of the positron and modern CERN experiments creating antihydrogen atoms.

Antimatéria

Frank Close

4.03(1179 Reviews)

Visão geral de Antimatéria

Mergulhe no enigmático mundo da antimatéria com o físico Frank Close, que desmistifica esta substância evasiva que alimenta exames de PET scan e desafia a nossa compreensão do universo. Além dos mitos da ficção científica, como os de "Anjos e Demônios", descubra a realidade fascinante da imagem espelhada da matéria.

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As mesmas ideias de Antimatéria. Escolha a voz, a profundidade e o ritmo ideais para você. Mude quando quiser.

Capítulo 1

When Matter Meets Its Mirror: The Explosive Reality of Antimatter

Imagine a substance so powerful that a gram of it could power an entire city for a year, yet so dangerous that it annihilates everything it touches in a flash of pure energy. This isn't science fiction-it's antimatter, the mysterious opposite of everything we know. Frank Close's "Antimatter" takes readers on a journey through one of physics' most fascinating frontiers, exploring a substance that sounds like it belongs in Star Trek but actually exists in laboratories today. Since the book's publication, antimatter has captured the public imagination, particularly after Dan Brown's "Angels and Demons" featured it as a doomsday weapon. Even NASA has invested millions researching antimatter propulsion, while CERN regularly produces tiny amounts for experiments. What makes this book particularly compelling is how it bridges the gap between speculative fiction and scientific reality, revealing that the truth about antimatter is both more mundane and more wondrous than Hollywood suggests.

Capítulo 2

The Explosive Encounter of Matter and Antimatter

What happens when an irresistible force meets an immovable object? This ancient philosophical puzzle points directly to antimatter-matter's topsy-turvy shadow where everything is reversed. When matter meets antimatter, they mutually annihilate in a blinding flash of energy, converting their entire mass into pure light according to Einstein's famous E=mc2. Antimatter isn't fiction-it's a scientific reality first predicted mathematically by Paul Dirac in 1928 and discovered experimentally just four years later. The positron-antimatter's version of the electron-appears identical to its matter counterpart except for having a positive rather than negative charge. Similarly, the antiproton mirrors the proton with negative rather than positive charge. Our universe appears to be the leftover remnant after a cosmic "Great Annihilation" following the Big Bang. Initially, matter and antimatter existed in perfect balance, but through processes scientists are still working to understand, a tiny imbalance developed-perhaps just one extra matter particle per ten billion pairs. When the universe cooled and the Great Annihilation occurred, this small excess of matter survived to form everything we see today. The energy released when matter meets antimatter is unmatched by anything else in nature. While chemical reactions release only about one-billionth of the available energy in matter, and nuclear reactions like those in atomic bombs liberate about one percent, antimatter annihilation releases 100% of the available energy. A kilogram of antimatter meeting a kilogram of matter would generate ten billion times more energy than a kilogram of TNT-enough to power an entire country for months. This extraordinary energy potential has made antimatter the power source of choice in science fiction and has inspired genuine NASA research programs. However, unlike fictional doomsday substances, antimatter's destructive potential is self-limiting-it destroys itself in the process of destroying matter, preventing chain reactions.

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Capítulo 3

The Mystery of the Tunguska Event

On June 30, 1908, something extraordinary happened in the remote Siberian wilderness near the Tunguska River. Witnesses described a blinding fireball that made sunlight appear dark by comparison, followed by a massive explosion visible from 700 kilometers away. The blast flattened trees like matchsticks across 2,000 square kilometers-an area the size of London-and created seismic waves detected around the globe. The explosion scattered so much dust into the atmosphere that it created unusual midnight twilight visible as far away as London. When scientist Leonid Kulik finally reached the site in 1927, he found a vast mud plain surrounded by charred tree stumps and fallen trees pointing outward from the epicenter-but crucially, no impact crater. Despite excavations to depths of 30 meters, no meteorite material was ever found. Scientists later calculated the explosion released nearly a million billion joules of energy-equivalent to an hour's energy consumption by the entire United Kingdom. This pattern of devastation without material remnants led some scientists to propose an intriguing theory: perhaps a small piece of antimatter, possibly as small as a meter across, had collided with Earth. Unlike a meteorite impact that would leave a crater and physical evidence, an antimatter collision would leave only a devastating explosion with no material remnants-exactly matching the Tunguska pattern. While later evidence has cast doubt on this theory, with most scientists now favoring the explanation of a comet fragment exploding in the atmosphere, the Tunguska event remains one of the most compelling potential antimatter encounters in Earth's history.

Capítulo 4

The Quantum World Where Antimatter Was Born

To truly understand antimatter, we must first explore the structure of ordinary matter itself. Our bodies consist of stardust-atoms forged in stars billions of years ago, organized into complex molecules like DNA. But the true distinction between matter and antimatter lies hidden at the subatomic level. Inside atoms, the fundamental difference becomes clear: electrical polarities are reversed. Where normal matter has positively charged nuclei and negatively charged electrons, antimatter has negatively charged nuclei and positively charged electrons. These opposing charges create mirror-image behaviors in electromagnetic interactions. The bizarre laws of the subatomic realm revealed the inevitability of antimatter's existence. Unlike Newton's deterministic laws governing visible objects, individual atoms follow quantum mechanics, which predicts only probabilities. This quantum world solved the paradox of atomic stability-classical physics predicted electrons should spiral into nuclei and destroy atoms instantly. Instead, quantum waves must fit precisely into electron orbits, like waves on a circular rope, preventing electrons from spiraling inward. Einstein's relativity revealed that matter is trapped energy. The famous equation E=mc2 demonstrates that even stationary objects contain energy within their atoms. For moving objects, the total energy combines rest energy and kinetic energy. This enables energy from light to transform into matter-but only as paired particles of opposite charge. When an electron emerges from light energy, its antimatter counterpart (the positron) must also appear, maintaining charge balance. The electron, which heralds the realm of antimatter, has both electric charge and twofold magnetism akin to a bar magnet. This magnetic property was revealed through the Zeeman effect, where spectral lines separated in a magnetic field. The electron appears to have an intrinsic "spin" that can be clockwise or anticlockwise-a property that remained mysterious until Dirac combined relativity and quantum mechanics in his groundbreaking equation.

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Capítulo 5

The Mathematical Genius Who Predicted Antimatter

Paul Dirac, son of a Swiss language teacher, was extraordinarily taciturn but mathematically brilliant. His classic text "The Principles of Quantum Mechanics" became the definitive work on the subject despite its challenging content. Dirac's famous equation, memorialized on his Westminster Abbey plaque near Newton's memorial, revealed the antiworld with mathematical elegance comparable to Shakespeare or Beethoven. Though famously uncommunicative in person-as illustrated by anecdotes with novelist E.M. Forster-Dirac expressed himself powerfully through mathematical symbols, creating an entirely new mathematical language that merged quantum theory with Einstein's special relativity. While Schrodinger's equation explained electron behavior in atoms at non-relativistic speeds, it couldn't account for electron spin. Dirac tackled this by developing a relativistic quantum equation using matrices instead of simple numbers. This mathematical innovation not only incorporated electron spin naturally but also produced solutions with both positive and negative energies-a puzzle that would lead to a revolutionary insight about the nature of particles and antiparticles. To resolve the paradox of negative energy states that would make matter unstable, Dirac proposed that what we call the vacuum is actually filled with an infinite "sea" of electrons occupying all possible negative energy states. This sea defines zero energy, and electrons cannot fall into negative states because they're already filled (following the exclusion principle). If energy knocks an electron from this sea, it leaves a "hole"-the absence of negative charge and negative energy appears as positive charge and positive energy. Initially, Dirac suggested the proton might be this "hole" in the electron sea, but Robert Oppenheimer pointed out this couldn't be correct since hydrogen atoms would self-destruct-matter would vanish in a flash of light upon electron-proton contact. Dirac accepted this criticism and in 1931 published that a "hole" would be "a new kind of particle...having the same mass and charge as an electron" which he called an "anti-electron." He proposed a "complete and perfect symmetry between positive and negative electric charge," predicting the antiproton and establishing the principle that every particle has an antiparticle counterpart-now recognized as a fundamental truth about our universe.

Capítulo 6

The Discovery of Antimatter in Cosmic Rays

High above Earth, cosmic rays from outer space crash into the atmosphere, creating showers of subatomic particles. Among these particles, scientists discovered the positron-the first evidence of antimatter's existence. Though positron tracks appeared in photographs as early as 1923, they weren't recognized until after Dirac's theoretical prediction. In 1923, Dmitry Skobeltzyn in Leningrad accidentally observed positron tracks while investigating gamma rays with a cloud chamber-a device that reveals particle paths through vapor trails. When he placed the chamber between magnetic poles to clear unwanted electrons, some particles curved "the wrong way." Though he showed these puzzling images at a 1928 Cambridge conference, no one recognized their significance. Carl Anderson at Caltech, using a more powerful magnet in 1930, discovered cosmic rays contained equal numbers of negative and positive particles. By placing a lead plate across his chamber, he proved these weren't upward-moving electrons but downward-moving "positive electrons." The name "positron" was coined in Science News Letter in December 1931. Patrick Blackett and Giuseppe Occhialini discovered that positrons were being created when cosmic rays hit their cloud chamber's copper plate. Their photographs showed up to twenty particle tracks diverging from points in the metal, with equal numbers of positive and negative particles. They realized that intense electric fields within copper atoms made passing electrons radiate gamma rays, which in turn produced pairs of electrons and positrons-demonstrating Einstein's E=mc2 by converting radiation into matter and antimatter. Once Dirac's theory and these discoveries spread, positrons were found everywhere in old cloud chamber photographs. The Joliot-Curies discovered radioactive nuclei that emit positrons-winning them the 1935 Nobel Prize for Chemistry. Unlike electrons that can flow as current or join neighboring atoms, positrons are strangers in our world of matter, quickly annihilating with electrons in a flash of light. This annihilation process has become key to practical applications, particularly in medicine. Positron emission tomography (PET) uses radioactive sugar molecules containing positron-emitting atoms to track brain activity. When positrons annihilate with electrons, the resulting gamma rays can be detected to create detailed brain images. Positron annihilation also helps detect metal fatigue in aircraft parts, and scientists have even created short-lived "positronium" atoms from electrons and positrons.

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Capítulo 7

The Subatomic Zoo: Quarks and Their Antimatter Twins

Beyond matter and antimatter exists a third category-things like electromagnetic radiation. Photons, from gamma rays to radio waves, represent this non-substance form. Matter and antimatter can annihilate into photons, and with enough energy, photons can transform into matter-antimatter pairs. These non-substantial particles are called "bosons" (after Satyendranath Bose), while matter and antimatter particles are "fermions" (after Enrico Fermi). Bosons transmit forces-photons carry electromagnetic force, gravitons (though undetected) likely carry gravity, gluons transmit the strong nuclear force, and W and Z bosons carry the weak force that enables the sun to shine by converting protons into helium, creating positrons in the process. Dirac's equation applies to all fermions, predicting antimatter counterparts for protons and neutrons. The antiproton has the same mass as a proton but negative charge, while the antineutron has zero charge but reversed internal electric currents and magnetism. After the positron's discovery, scientists sought the antiproton, which required much more energy to create. The BeVatron accelerator at Berkeley was built specifically for this purpose, and in 1955 a team led by Chamberlain and Segre announced the discovery. The antineutron followed in 1957. By the 1950s, particle accelerators had revealed a bewildering array of particles beyond the simple electron, proton, and neutron. Donald Glaser's bubble chamber invention in 1952 helped visualize these particles' trails. Scientists gradually discerned patterns among these particles, similar to Mendeleev's Periodic Table. Experiments at Stanford revealed that protons and neutrons aren't elementary but contain smaller particles called quarks. Protons contain two "up" quarks (+2/3 charge each) and one "down" quark (-1/3 charge), while neutrons contain one up and two downs. Adding a third type, the "strange" quark, explains the many "strange" particles discovered. Each quark has an antiquark counterpart with opposite charge, allowing the formation of antiprotons, antineutrons, and other antimatter particles. The strong force can bind not only trios of quarks or antiquarks but also quark-antiquark pairs, creating particles like pions and kaons that are neither purely matter nor antimatter. These combinations are extremely short-lived as the quark and antiquark quickly annihilate each other.

Capítulo 8

The Ingenious Challenge of Storing the Unstoppable

How do you store something that destroys everything it touches? This fundamental challenge of antimatter containment required ingenious solutions using magnetic and electric fields rather than physical containers. Bruno Touschek solved the antimatter storage problem by creating a "cage without material walls"-a vacuum better than outer space with magnetic and electric fields confining antimatter particles in circulating beams. At CERN, a 27-kilometer ring of magnets guided positrons at near light-speed for weeks. In 1960, Touschek built on Rolf Wideroe's earlier work on particle acceleration to create a breakthrough: instead of using two sets of magnets to send particles in opposite directions, he realized one set could simultaneously steer electrons one way and positrons the other. His team built ADA (Anello d'Accumulazione), a mere meter in diameter, which successfully stored both electrons and positrons-the first time antimatter had been tamed. Storing antiprotons presented greater challenges than positrons due to their much greater mass. While creating antiprotons was achievable (first done in 1955), controlling them proved difficult as they would escape magnetic fields and annihilate against container walls. Gersh Budker pioneered "cooling" them by passing antiprotons through clouds of electrons, transferring their erratic energy to the electrons. In 1979, Carlo Rubbia at CERN planned to produce W and Z particles through proton-antiproton annihilations. Dutch engineer Simon van der Meer solved the crucial problem with his "Antiproton Accumulator" (AA), which cooled antiprotons into well-behaved beams. His ingenious insight: signals could be sent across the diameter of the ring faster than particles traveled around the semicircle, allowing time for electronic corrections. In 1984, Hans Dehmelt achieved a breakthrough by storing a single positron for three months in a device half the size of a human thumb. Building on Frans Penning's 1930s work with vacuum tubes, Dehmelt created the "Penning trap"-an ingenious combination of electric and magnetic fields that could trap particles indefinitely. By creating a hollow cylindrical anode with cathodes at angles on the top and bottom, he effectively made a canister of electric and magnetic fields rather than metal. While positrons were relatively easy to trap, antiprotons presented greater challenges due to their larger mass and energy. Gerald Gabrielse took up the challenge of capturing antiprotons from CERN's Low Energy Antiproton Ring (LEAR). By 1986, he had captured antiprotons in his 15-centimeter trap, and by 1995 achieved the goal of isolating a single antiproton.

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Capítulo 9

Creating Antimatter Atoms: The Ultimate Challenge

Creating stable antimatter atoms presented unique challenges since neutral atoms can't be contained by electric and magnetic fields. In 1995, CERN produced the first handful of antihydrogen atoms in history, though they existed for only fractions of a second before annihilation. After LEAR's operation ended in 1996, the Antiproton Decelerator (AD) was built specifically for antimatter production. The ATHENA experiment captured thousands of antiprotons from the AD, slowed them dramatically, and mixed them with millions of cold positrons to form antihydrogen. Detection occurred when these neutral anti-atoms escaped the trap and annihilated with normal matter. By 2002, ATHENA and ATRAP were producing tens of thousands of antihydrogen atoms. The successor experiment ALPHA achieved a major breakthrough in 2011 by trapping antihydrogen for 16 minutes, enabling the first studies of antimatter properties. In 2013, ALPHA demonstrated that antihydrogen falls under normal gravity, and by 2017 had measured its hyperfine transition, finding it identical to hydrogen within experimental accuracy. The Large Electron Positron collider (LEP) was an engineering marvel of such precision that it detected the moon's gravitational effect on Earth's crust, which altered the ring's circumference by millimeters throughout the lunar cycle. This affected beam timing by nanoseconds on a 28-day cycle. LEP became the birthplace of the World Wide Web, invented to facilitate instant data sharing among hundreds of collaborating scientists. During its decade of operation, LEP revealed how matter emerged when the universe was just a billionth of a second old, producing pairs of particles and antiparticles. Beyond the familiar electron and quarks, LEP confirmed heavier versions-the muon (200 times heavier than an electron) and tau (4,000 times heavier), each with its own antiparticle. Similarly, the up and down quarks that form protons and neutrons have heavier counterparts: charm and top (for up), and strange and bottom (for down).

Capítulo 10

The Cosmic Asymmetry: Why Matter Prevailed

The relationship between antimatter and time forms a profound symmetry at the heart of physics. Richard Feynman's famous diagrams, which revolutionized particle physics calculations, built upon Ernst Stueckelberg's earlier insight that antiparticles could be viewed mathematically as particles traveling backward in time. This doesn't mean antimatter actually moves backward through time, but rather illustrates a fundamental symmetry in physics equations. At the elementary particle level, the laws of physics remain unchanged when three properties are simultaneously reversed: charge (C), parity/mirror symmetry (P), and time (T). This CPT symmetry reveals antimatter's true nature as matter's perfect counterpart. The symmetry between matter and antimatter, reminiscent of the yin-yang concept, proves imperfect upon closer inspection. The neutral kaon (K0), composed of a down quark and strange antiquark, revealed this asymmetry in a groundbreaking 1964 experiment by Cronin and Fitch. Unlike most particles, K0 and its antiparticle continuously transform into each other through a quantum Jekyll-and-Hyde oscillation. CERN experiments in 1998 proved that anti-K0 transforms into K0 slightly faster than the reverse process, demonstrating a fundamental time asymmetry at the particle level. This means if you start with equal amounts of K0 and anti-K0, a small excess of K0 eventually develops-insufficient to explain the universe's matter dominance, but proof that such asymmetry can naturally arise. How would you determine if aliens on a distant planet were made of matter or antimatter? Since both sides would insist they're made of "matter," we need an objective test. The asymmetry between matter and antimatter provides the answer. The long-lived neutral K meson offers a definitive test: in our matter world, when it decays, it produces a positron slightly more often than an electron (1,003 versus 997 per 2,000 decays). By discussing this particle with aliens and asking which lightweight decay product appears most frequently, we can determine their composition without risking annihilation through direct contact.

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Capítulo 11

The Elusive Promise of Antimatter Technology

The biggest mystery surrounding antimatter is its scarcity in our universe. If the Big Bang created matter and antimatter in equal amounts, they should have annihilated each other immediately, leaving nothing but energy. The question becomes not why antimatter disappeared, but why matter survived at all. Though antihydrogen atoms exist, theory suggests entire anti-elements and even anti-life could form with identical chemistry to normal matter. But where is all this antimatter? We know our solar system contains none-the moon landings confirmed this, and any anticomets would produce massive gamma ray bursts when hitting the solar wind. Evidence indicates our observable universe is dominated by matter, with approximately one proton per five cubic meters of space. The leading theory suggests that immediately after the Big Bang, there were ten billion each of radiation quanta, protons and antiprotons, plus one extra proton for every ten billion pairs-this tiny imbalance survived the "Great Annihilation" to form our matter universe. Neutrinos may hold the key to the mystery of missing antimatter. These ghostly particles have no electric charge, minimal mass, and can pass through Earth effortlessly. Unlike photons, neutrinos are fermions that obey Dirac's equation and distinguish between matter and antimatter. Recent discoveries that neutrinos have tiny mass have enormous implications, as it means they can switch between left and right-handed spin. Ettore Majorana's theory that neutrinos might be both matter and antimatter could explain our matter-dominated universe. Despite reports of US Air Force antimatter weapons development, the reality makes such applications impossible. Current technology might produce a nanogram of antimatter yearly at a cost of tens of millions of dollars, meaning a single gram would require hundreds of millions of years and over $1,000 trillion. While antimatter spacecraft propulsion seems theoretically attractive-potentially reducing a Mars mission's three tonnes of chemical propellant to just a hundredth of a gram of antimatter-the containment challenges remain insurmountable. Gerald Smith's team from Penn State University proposed a development program in the 1990s, confidently planning traps capable of carrying 1014 antiprotons for Mars missions. A decade later, these ambitions remain unrealized-the maximum ever stored is just a million antiprotons. While antimatter will never be practical for large-scale energy production, its annihilation has proven invaluable in medicine, technology, and fundamental science. When particle beams collide at near light-speed, the energy concentration in a volume smaller than an atomic nucleus is enormous. Most significantly, antiproton and positron beams have enabled scientists to simulate conditions of the early universe less than a billionth of a second after the Big Bang. This represents a profound achievement of human intellect-groups of atoms organized into beings capable of building machines that revisit the origins of the universe itself.

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Temas principais em Antimatéria

particle annihilation
matter-antimatter asymmetry
quantum electrodynamics
subatomic mirror images
energy conversion

Citações de Antimatéria

Matter is trapped energy.
Our bodies consist of stardust.
Antimatter isn't fiction-it's a scientific reality.
The electron, which heralds the realm of antimatter, has both electric charge and twofold magnetism.
Dirac expressed himself powerfully through mathematical symbols.

Personagens de Antimatéria

Frank CloseAuthor and physicist exploring antimatter
Paul DiracPhysicist who mathematically predicted antimatter
Leonid KulikScientist who investigated the Tunguska event

Sobre o Autor

Frank Close é um físico de partículas e professor emérito de física na Universidade de Oxford, renomado por tornar conceitos científicos complexos acessíveis através de livros como Antimatéria. Membro da Royal Society e agraciado com a Medalha Kelvin, Close combina décadas de pesquisa sobre partículas subatômicas com uma narrativa lúcida para explorar questões fundamentais sobre os blocos de construção do universo. Sua expertise abrange física teórica, história da ciência e comunicação pública — incluindo cargos como chefe de comunicações no CERN e vice-presidente da British Science Association.

Outras obras notáveis de Close incluem The Infinity Puzzle, que narra a busca pelo bóson de Higgs, e Elusive: How Peter Higgs Solved the Mystery of Mass, um mergulho biográfico profundo na pesquisa vencedora do Prêmio Nobel.

Seus mais de 20 livros, traduzidos para 19 idiomas, unem o rigor acadêmico à curiosidade do grande público. Close foi condecorado com um OBE em 2000 por promover a compreensão pública da ciência, consolidando seu status como uma voz líder na educação em física. Antimatéria reflete sua mistura característica de narrativa histórica e teoria de ponta, desmistificando um dos fenômenos mais enigmáticos do universo.

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@SofiaP

"BeFreed replaced my podcast queue. Imagine Spotify for books — that’s it. 🙌"

@Jaded_Falcon

201

"It is great for me to learn something from the book without reading it."

@OojasSalunke

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@Leo, Law Student, UPenn

483

"Makes me feel smarter every time before going to work"

@Cashflowbubu

"Instead of endless scrolling, I just hit play on BeFreed. It saves me so much time."

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117

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@Raaaaaachelw

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483

"Makes me feel smarter every time before going to work"

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Capítulo 11

Antimatéria

Visão GeralVisão geral de Antimatéria

Um livro. Muitas maneiras de ouvi-lo.

When Matter Meets Its Mirror: The Explosive Reality of Antimatter

The Explosive Encounter of Matter and Antimatter

Veja cada palavra enquanto a ouve

The Mystery of the Tunguska Event

The Quantum World Where Antimatter Was Born

Aproveite ainda mais Antimatéria

The Mathematical Genius Who Predicted Antimatter

The Discovery of Antimatter in Cosmic Rays

Veja cada palavra enquanto a ouve

The Subatomic Zoo: Quarks and Their Antimatter Twins

The Ingenious Challenge of Storing the Unstoppable

Aproveite ainda mais Antimatéria

Creating Antimatter Atoms: The Ultimate Challenge

The Cosmic Asymmetry: Why Matter Prevailed

Veja cada palavra enquanto a ouve

The Elusive Promise of Antimatter Technology

Você chegou ao fim de Antimatéria

Temas principais em Antimatéria

Citações de Antimatéria

Personagens de Antimatéria

Sobre o Autor

Baixar resumo de Antimatéria

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Perguntas Frequentes Sobre Este Livro

What is Antimatter by Frank Close about?

Who should read Antimatter by Frank Close?

Is Antimatter by Frank Close worth reading?

What is the Dirac equation, and why is it important in Antimatter?

Descubra mais

1,000,000+ curious minds.

1,000,000+ curious minds.

Um livro. Muitas maneiras de ouvi-lo.

When Matter Meets Its Mirror: The Explosive Reality of Antimatter

The Explosive Encounter of Matter and Antimatter

Veja cada palavra enquanto a ouve

The Mystery of the Tunguska Event

The Quantum World Where Antimatter Was Born

Aproveite ainda mais Antimatéria

The Mathematical Genius Who Predicted Antimatter

The Discovery of Antimatter in Cosmic Rays

Veja cada palavra enquanto a ouve

The Subatomic Zoo: Quarks and Their Antimatter Twins

The Ingenious Challenge of Storing the Unstoppable

Aproveite ainda mais Antimatéria

Creating Antimatter Atoms: The Ultimate Challenge

The Cosmic Asymmetry: Why Matter Prevailed

Veja cada palavra enquanto a ouve

The Elusive Promise of Antimatter Technology

Você chegou ao fim de Antimatéria

Usuários também gostaram

Descubra mais

Visão geral de Antimatéria