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ویرایش: 1
نویسندگان: Rabindra N. Mohapatra
سری:
ISBN (شابک) : 9783030518455, 9783030518462
ناشر: Springer
سال نشر: 2021
تعداد صفحات: 219
زبان: English
فرمت فایل : PDF (درصورت درخواست کاربر به PDF، EPUB یا AZW3 تبدیل می شود)
حجم فایل: 4 مگابایت
در صورت تبدیل فایل کتاب The neutrino story: One tiny particle’s grand role in the cosmos به فرمت های PDF، EPUB، AZW3، MOBI و یا DJVU می توانید به پشتیبان اطلاع دهید تا فایل مورد نظر را تبدیل نمایند.
توجه داشته باشید کتاب داستان نوترینو: نقش بزرگ یک ذره کوچک در کیهان نسخه زبان اصلی می باشد و کتاب ترجمه شده به فارسی نمی باشد. وبسایت اینترنشنال لایبرری ارائه دهنده کتاب های زبان اصلی می باشد و هیچ گونه کتاب ترجمه شده یا نوشته شده به فارسی را ارائه نمی دهد.
هر ثانیه در هر روز، ما در معرض میلیاردها نوترینو ساطع شده از خورشید قرار میگیریم، و با این حال به نظر میرسد که آنها مستقیماً از ما عبور میکنند و اصلاً هیچ اثر ظاهری ندارند. این ذره زیر اتمی ممکن است کوچک و ضعیف باشد، اما این کتاب به شما نشان می دهد که چقدر نقش مهمی در تکامل عناصر جهان و در نهایت خودمان داشته است. ابتدا با مقدمهای بر مبانی فیزیک زیراتمی، از جمله پیشزمینههای مختصر در مورد اکتشافاتی که زمینه را برای پیشرفتهای بزرگ قرن بیستم فراهم کردند، شروع میکنیم. نویسنده، یک فیزیکدان نظری برجسته که بیش از سی سال در مورد نوترینوها تحقیق کرده است، در ادامه به زبان غیر فنی توضیح می دهد که چگونه و چرا نوترینو در داستان گسترده تر ذرات بنیادی قرار می گیرد. در نهایت، خواننده با آخرین اکتشافات در نیم قرن گذشته مطالعات نوترینو آشنا خواهد شد. این کتاب علمی نیمه محبوب برای هر دانشجوی فیزیک یا فیزیکدان غیرمتخصصی که مایل به دانستن بیشتر در مورد نوترینو و نقش آن در تکامل جهان ما هستند، جذاب خواهد بود.
Every second of every day, we are exposed to billions of neutrinos emitted by the Sun, and yet they seem to pass straight through us with no apparent effect at all. Tiny and weakly interacting this subatomic particle may be, but this book will show you just how crucial a role it has played in the evolution of the elements in the universe, and eventually, ourselves. We first start with an introduction to the basics of subatomic physics, including brief backgrounds on the discoveries that set the stage for major 20th century advances. The author, a distinguished theoretical physicist who has researched neutrinos for over thirty years, next explains in nontechnical language how and why the neutrino fits into the wider story of elementary particles. Finally, the reader will learn about the latest discoveries in the past half century of neutrino studies. This semi-popular science book will appeal to any physics students or non-specialist physicists who wish to know more about the neutrino and its role in the evolution of our universe.
Preface Acknowledgements Contents Part I 1 Introduction 2 Particles as Building Blocks of Matter 2.1 Protons and Electrons 2.2 Add the Neutron 2.3 Particle Spin 2.4 Particle Helicity 2.5 Stable and Unstable Particles 2.6 Matter and Anti-Matter from Einstein\'s Theory of Relativity: The Power of an Algebraic Sign 3 From Protons and Neutrons to a Zoo of Particles 3.1 Looking Inside Protons and Neutrons with High Energy Colliders 3.2 Particles from Cosmic Rays 4 Order in the Zoo and Quarks 4.1 Eightfold Way and Quarks Inside Baryons and Mesons 4.2 Baryons Have Their Own Markers, the Baryon Number (B) 4.3 Leptons Have Their Own Marker Too: The Lepton Number (L) 5 Forces That Keep the Universe Together 5.1 Gravity 5.2 Black Holes and Gravity 5.3 Electromagnetic Force 5.4 Nuclear Force 5.5 Weak Force 6 Forces Are Also Caused by Particles 6.1 Photon, Mesons, and Forces 6.2 Had the Force Strengths Been Different? Part II 7 The Neutrino Is Born as an Idea 7.1 Missing Energy Puzzle in Beta Ray Emission 7.2 December Night Ball and Pauli Letter 8 From Idea to Reality: The Neutrino Story Unfolds in Slow Motion 8.1 Fermi Theory of Beta Decay 8.2 Can the Neutrino Be Found? 9 The Neutrino is Discovered 9.1 How to Detect a Neutrino 9.2 From Hanford to Savanna River 9.3 The Years That Followed the Neutrino Discovery 9.4 More Neutrino Types Found 9.5 Charged Weak Force Comes Accompanied by Neutral Weak Force 10 Standard Model of the Particles and Forces 10.1 How Charming was the Charm Quark? 10.2 The Quark Family and Their Interaction 10.3 Leptons and the Monogamous Neutrinos 11 Forces in the Standard Model and Symmetries 11.1 Are the Weak Forces Also from Gauge Symmetry Like the Electric Force? 11.2 Where Did Mass Come from? 11.3 Symmetries and Symmetry Breaking 11.4 Spontaneous Symmetry Breaking 11.5 Higgs Mechanism 11.6 The Theory of Strong Force 12 More Physics Beyond the Standard Model or the End of Physics Now? 12.1 Future Colliders and New Physics 12.2 Non-Accelerator Probes of Physics Beyond the Standard Model 13 Neutrinos Oscillate and Hence They Weigh 13.1 From Oscillating Swing to Oscillating Neutrino 13.2 Quantum Mechanics and Neutrino Oscillations 13.3 Detecting Neutrino Oscillations 13.4 Ray Davis and Catching of Solar Neutrinos 13.5 Super-Kamiokande Experiment 13.6 Atmospheric Neutrino Oscillation 13.7 Neutrino Oscillations Confirmed by Accelerator and Reactor Neutrinos 13.8 Understanding the Sun Using Solar Neutrinos 14 What Have We Learned about Neutrinos from Neutrino Oscillation Experiments? 14.1 Who Is Heavy and Who Is Light: Mass Ordering of Neutrinos 14.2 Refraction of Neutrinos in Matter 14.3 Do Neutrinos Decay? 14.4 Long Distance Communication Using Neutrinos 14.5 Using Neutrinos for National Security Purpose 14.6 Worldwide Effort to a Fuller Understanding of Neutrino Mass 14.7 Can Neutrino Be Sensitive to Magnetic Forces: The Neutrino Magnetic Moment 14.8 What Oscillation Experiments Do Not Tell Us Part III 15 Mendeleev\'s Periodic Table 16 A Brief Overview of the Big Bang Theory of the Universe 16.1 Big Bang Theory vs. Steady State Theory 16.2 Big Bang Theory Wins 16.3 Major Events in the Universe\'s Past 17 The Inflationary Universe 17.1 Inflation: One Beginning Before Another Beginning 17.2 Beginning of the Hubble Era after Inflation 18 From Quarks to Protons and Neutrons and Then to Helium and Beryllium and the Dance of Atoms 18.1 Big Bang Nucleosynthesis 18.2 Formation of Galaxies 18.3 Cosmic Microwave and Neutrino Backgrounds 19 Stars as the Cooking Pots for Heavy Nuclei 19.1 Stellar Nucleosynthesis 19.2 Still Heavier Elements 20 Neutrino Mass Hints at Mirror Symmetry in Nature 20.1 Back to Symmetries 20.2 Mirror Symmetry and Weak Force 20.3 Mirror Symmetry and Neutrinos 20.4 Mass and Helicity 20.5 Mirror Reflection and Neutrino States and Nature of Weak Force 21 Mirror Symmetric Weak Force and Neutrino Mass 21.1 Neutrino Mass-Mirror Symmetry Breaking Connection 21.2 Majorana Neutrinos 21.3 Seesaw and Majorana Neutrino Mass 21.4 Testing Majorana Nature of Neutrinos in Experiments 22 Hints of Other New Physics from Neutrino Mass 22.1 Mirror Universe Versus Left–Right Symmetry: Two Paths to Parity 22.2 Grand Unification of Forces and Matter 22.3 What if Neutrinos Are not Majorana Fermions? 23 The Origin of Matter and Neutrinos 23.1 Enter Sakharov 23.2 The Search for Baryon Number Violation 23.3 Neutrino Seesaw and Baryon Asymmetry 24 Dark Universe 24.1 Dark Matter and Galaxies 24.2 What is the Dark Matter? 24.3 Is There a Parallel Universe? 24.4 Are There Sterile Neutrinos? 24.5 Can We Communicate with the Mirror World? 25 Neutrinos from Heavenly Sources 25.1 Why Look for Neutrinos from Extra-Solar Sources and Extra-Galactic Sources 25.2 Supernova Neutrinos 25.3 Neutrinos Observed in the IceCube Experiment in the South Pole Part IV 26 Anthropic Principle 26.1 Why Go Anthropic? 26.2 Many Universes and the Anthropic Principle 26.3 Other Examples 27 What Lies Ahead? 27.1 ``Near\'\' Future: The First Ten Billion (1010) Years 27.2 One Hundred Billion Billion (1020) Years 27.3 Far Future: Beyond the Next Million Trillion Trillion Years 1030 Years 28 Epilogue References Index