Best of NASA: Landmark "Ghost Particle" Detection in 4k
For more 4K space, and more great History and Science than you'll ever watch, check out our sister network... https://www.magellantv.com/featured High-energy neutrinos are hard-to-catch particles that scientists think are created by the most powerful events in the cosmos, such as galaxy m
From playlist SpaceRip 4K
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From playlist Science Unplugged: Neutrinos
The Elusive Neutrino and The Nature Of The Cosmos
The neutrino is among the cagiest of particles, a subatomic wisp so ephemeral it could pass through light years of lead with more ease than a hot knife through butter. Despite its extraordinary abundance in the universe—billions pass through your body every second—this ghostly particle is
From playlist Neutrinos
Why I Love Neutrinos - Elena Gramellini
Why I Love Neutrinos is a series spotlighting those mysterious, abundant, ghostly particles that are all around us. This installment features Yale Graduate Student Elena Gramellini. For more information on neutrinos, visit the Fermilab website at http://www.fnal.gov.
From playlist Why I Love Neutrinos
Why I Love Neutrinos is a series spotlighting those mysterious, abundant, ghostly particles that are all around us. This installment features a compilation of international scientists. For more information on neutrinos, visit the Fermilab website at http://www.fnal.gov.
From playlist Why I Love Neutrinos
From playlist Courses and Series
Teach Astronomy - Evidence for Cosmic Acceleration
http://www.teachastronomy.com/ The primary evidence that the universe is currently accelerating comes from distant supernovae. The observation is based on the fact that a standard cosmology filled with only radiation and matter, most of which is dark matter, predicts the brightness of dis
From playlist 22. The Big Bang, Inflation, and General Cosmology
Detecting Cosmic Neutrinos with IceCube at the Earth's South Pole - Naoko Kurahashi Nielson
Naoko Kurahashi Nielson Drexel University March 10, 2015 ABSTRACT: The IceCube Neutrino Observatory has recently discovered a diffuse flux of astrophysical neutrinos, neutrinos from beyond the solar system. But how does one collect neutrinos at the South Pole? Why study neutrinos for astr
From playlist Joint IAS/PU Astrophysics Colloquium
From playlist Courses and Series
Christian Ott: Modeling the Death of Massive Stars
PROGRAM: NUMERICAL RELATIVITY DATES: Monday 10 Jun, 2013 - Friday 05 Jul, 2013 VENUE: ICTS-TIFR, IISc Campus, Bangalore DETAL Numerical relativity deals with solving Einstein's field equations using supercomputers. Numerical relativity is an essential tool for the accurate modeling of a wi
From playlist Numerical Relativity
JWST Worth the Hype? How to Build a Wormhole? How to Pass Van Allen Belts? | Q&A 195
Are there alternatives to CMB? Will we ever build a space elevator? How can we see radiation coming from a black hole when nothing can escape it? Can you heat something with gravitational waves? Why JWST can look lame to the laymen? All this and more in this week's Q&A with Fraser Cain. 🦄
From playlist Questions and Answers with Fraser Cain
Miguel Ángel Aloy - magnetic fields & rotation of massive stars in their compact remnants
Recorded 5 October 2021. Miguel Ángel Aloy of the University of Valencia presents "Assessing the dependence of magnetic fields and rotation of massive stars in the properties of their compact remnants" at IPAM's Workshop I: Computational Challenges in Multi-Messenger Astrophysics. Abstract
From playlist Workshop: Computational Challenges in Multi-Messenger Astrophysics
Neutrino Quantum Kinetics in Neutron Star Mergers - Sherwood Richers III
Topic: Neutrino Quantum Kinetics in Neutron Star Mergers Speaker: Sherwood Richers III Affiliation: University of California, Berkeley Date: May 12, 2022 Following the collision of two compact objects, an accretion disk forms and from it matter is ejected that sources the universe's heavy
From playlist Astrophysics Seminar
The Surprisingly Dynamic...Massive Stars - Eliot Quataert
Joint IAS/Princeton University Astrophysics Colloquium Tuesday, October 27, 2015 http://www.sns.ias.edu/~seminar/colloquia.shtml In the last few years of the lives of massive stars, fusion in the core of the star produces a nuclear power that greatly exceeds the Eddington luminosity. Thi
From playlist Joint IAS/PU Astrophysics Colloquium
Irene Di Palma - A Machine Learning Application in Multi-Messenger Astrophysics - IPAM at UCLA
Recorded 7 October 2021. Irene Di Palma of the Sapienza University of Rome presents "A Machine Learning Application in Multi-Messenger Astrophysics" at IPAM's Workshop I: Computational Challenges in Multi-Messenger Astrophysics. Abstract: The detection of gravitational waves from core-coll
From playlist Workshop: Computational Challenges in Multi-Messenger Astrophysics
Supernova Neutrinos by Sovan Chakravarty
DISCUSSION MEETING PARTICLE PHYSICS: PHENOMENA, PUZZLES, PROMISES ORGANIZERS: Amol Dighe, Rick S Gupta, Sreerup Raychaudhuri and Tuhin S Roy, Department of Theoretical Physics, TIFR, India DATE: 21 November 2022 to 23 November 2022 VENUE: Ramanujan Lecture Hall and Online While the LH
From playlist Particle Physics: Phenomena, Puzzles, Promises - (Edited)
Neutrinos: Messengers from a Violent Universe
In this 45-minute presentation Alex Himmel, Wilson Fellow at Fermi National Accelerator Laboratory, explains how neutrinos might provide the answers to many questions that scientists have about the universe. The neutrino is a type of subatomic particle. They are produced in copious quantit
From playlist Neutrinos
The Alchemy of Neutron Star Collisions
PBS Member Stations rely on viewers like you. To support your local station, go to: http://to.pbs.org/DonateSPACE ↓ More info below ↓ Carl Sagan’s famous words: “We are star stuff” refers to a mind-blowing idea – that most atomic nuclei in our bodies were created in the nuclear furnace an
From playlist Neutron Stars Explained!
Teach Astronomy - Microwave Background Dipole
http://www.teachastronomy.com/ The cosmic microwave background radiation is generally smooth, and it's generally at the same temperature in every direction in the sky. But it's not perfectly smooth, and it's not at exactly the same temperature. The radiation is slightly warmer or blueshi
From playlist 22. The Big Bang, Inflation, and General Cosmology
Anthony Mezzacappa - Computational Challenges with Modeling Core Collapse Supernovae - IPAM at UCLA
Recorded 4 October 2021. Anthony Mezzacappa of the University of Tennessee presents "The Computational Challenges associated with Modeling Core Collapse Supernovae and their Gravitational Wave Emission" at IPAM's Workshop I: Computational Challenges in Multi-Messenger Astrophysics. Abstrac
From playlist Workshop: Computational Challenges in Multi-Messenger Astrophysics