A neutrino is a subatomic particle that is very similar to an electron, but has no electrical charge and a very small mass, which might even be zero. Neutrinos are one of the most abundant. Neutrino — the core player for the Mac with advanced playback features you won't find in any other player. Add effects, reverb, loops, time, pitch, Audio Units plug-ins, and more, all in real time. Enhance your music with equalizers and space correcting audio units. Explore stunning Music Visualizer representations of your music as it plays. Screenshot for Neutrino (was AudioCodex) Bad Link Rating: 1 (1 votes) AudioCodex is an alternative media player for Mac OS X that tightly integrates your media, iTunes Library, Quartz Compositions and Core Audio effects. AudioCodex is made for musicians, DJ/VJs, audiophiles and casual listeners alike. Requirements: OS X 10.6.8 - 10.8.
One outstanding Mac OS X issue unrelated to hubs is that Mac OS X versions prior to 10.8.5 do not support USB 3.0 audio devices. There are rumors Apple will resolve this issue in 10.8.5. Currently, working around this issue by connecting USB Audio devices to a USB 2.0 hub is our only available workaround.
NEUTRINO TRAILS.When a neutrino hits the heavy water in the detector's spherical vessel, a cone of light--here clearly visible in red--spreads out to sensors surrounding the device. The neutrinos detected in this event are probably muon-neutrinos, produced when cosmic rays strike the earth's atmosphere. |
A neutrino is a subatomic particle that is very similar to an electron, but has no electrical charge and a very small mass, which might even be zero. Neutrinos are one of the most abundant particles in the universe. Because they have very little interaction with matter, however, they are incredibly difficult to detect. Nuclear forces treat electrons and neutrinos identically; neither participate in the strong nuclear force, but both participate equally in the weak nuclear force. Particles with this property are termed leptons. In addition to the electron (and it's anti-particle, the positron), the charged leptons include the muon (with a mass 200 times greater than that of the electron), the tau (with mass 3,500 times greater than that of the electron) and their anti-particles.
Both the muon and the tau, like the electron, have accompanying neutrinos, which are called the muon-neutrino and tau-neutrino. The three neutrino types appear to be distinct: For instance, when muon-neutrinos interact with a target, they will always produce muons, and never taus or electrons. In particle interactions, although electrons and electron-neutrinos can be created and destroyed, the sum of the number of electrons and electron-neutrinos is conserved. This fact leads to dividing the leptons into three families, each with a charged lepton and its accompanying neutrino.
Neutrino Mac版
To detect neutrinos, very large and very sensitive detectors are required. Typically, a low-energy neutrino will travel through many light-years of normal matter before interacting with anything. Consequently, all terrestrial neutrino experiments rely on measuring the tiny fraction of neutrinos that interact in reasonably sized detectors. For example, in the Sudbury Neutrino Observatory, a 1000 ton heavy water solar-neutrino detector picks up about 1012Neutrino For Mac Download
neutrinos each second. About 30 neutrinos per day are detected.FAINT EVIDENCE. In this solar neutrino event, 75 of the 9,600 light sensors in the detector observed a photon of light. Lines trace the path from the neutrino's impact with heavy water to the light sensors. |
Wolfgang Pauli first postulated the existance of the neutrino in 1930. At that time, a problem arose because it seemed that both energy and angular momentum were not conserved in beta-decay. But Pauli pointed out that if a non-interacting, neutral particle--a neutrino--were emitted, one could recover the conservation laws. The first detection of neutrinos did not occur until 1955, when Clyde Cowan and Frederick Reines recorded anti-neutrinos emitted by a nuclear reactor.
Natural sources of neutrinos include the radioactive decay of primordial elements within the earth, which generate a large flux of low-energy electron-anti-neutrinos. Calculations show that about 2 percent of the sun's energy is carried away by neutrinos produced in fusion reactions there. Supernovae too are predominantly a neutrino phenomenon, because neutrinos are the only particles that can penetrate the very dense material produced in a collapsing star; only a small fraction of the available energy is converted to light. It is possible that a large fraction of the dark matter of the universe consists of primordial, Big Bang neutrinos.
The fields related to neutrino particles and astrophysics are rich, diverse and developing rapidly. So it is impossible to try to summarize all of the activities in the field in a short note. That said, current questions attracting a large amount of experimental and theoretical effort include the following: What are the masses of the various neutrinos? How do they affect Big Bang cosmology? Do neutrinos oscillate? Or can neutrinos of one type change into another type as they travel through matter and space? Are neutrinos fundamentally distinct from their anti-particles? How do stars collapse and form supernovae? What is the role of the neutrino in cosmology?
One long-standing issue of particular interest is the so-called solar neutrino problem. This name refers to the fact that several terrestrial experiments, spanning the past three decades, have consistently observed fewer solar neutrinos than would be necessary to produce the energy emitted from the sun. One possible solution is that neutrinos oscillate--that is, the electron neutrinos created in the sun change into muon- or tau-neutrinos as they travel to the earth. Because it is much more difficult to measure low-energy muon- or tau-neutrinos, this sort of conversion would explain why we have not observed the correct number of neutrinos on Earth.
Neutrino is a free plug-in that offers a glimpse into iZotope’s newest mixing technology. Insert Neutrino on multiple tracks across your session to reveal a subtle amount of detail that can help elevate great mixes to a new level of refinement.
Based on iZotope’s Spectral Shaping technology, Neutrino listens to your audio and provides subtle, real-time adjustments based on perceptual hearing models to reduce momentary unevenness in a signal transparently, in a way that conventional equalizers and compressors cannot. With simple controls and low-CPU usage, you can put it on every track in your session and achieve better-balanced mixes without sacrificing dynamics and sonic integrity. Best of all, it’s free to download, and easy to use.
Features
- Clarity across the board: Ultra efficient and designed to add unprecedented balance and focus to a mix when applied to every track, conceptually similar to analog summing or console emulations.
- Four modes for tailored response: Voices have a completely different sonic character, dynamic range, and frequency response than drums, bass, and other instruments. Shouldn’t your processing take that into account?
- Voice Mode focuses processing on mid and high frequencies for adding clarity and detail that helps vocals sit on top of the mix without becoming harsh or strident.
- Instrument Mode smoothes resonant frequencies while preserving the authentic character of the instrument.
- Bass Mode is designed to attenuate notes that stick out while adding punch and weight to electric, acoustic, and synth basses.
- Drum Mode emphasizes transient detail across the spectrum while minimizing frequency build-ups that can sound “muddy” or “flabby.”
- Simple controls: Tweak just two knobs to dial in the appropriate processing amount and detail for your music.
System Requirements
Supported operating systems
- Windows: 7, 8, and 10
- Mac: OS X 10.9–10.11
Plug-in formats
Neutrino For Pc
- VST 2 (32-bit and 64-bit), VST 3 (32-bit and 64-bit), Audio Unit (32-bit and 64-bit), AAX (64-bit), RTAS (32-bit), Audiosuite DPM and AAX.
Plug-in host compatibility
Neutrino Mac 使い方
- Logic Pro X.2, Ableton Live 9.5, Pro Tools 12.4, Pro Tools 11.3.1, Cubase Pro 8.5, REAPER 5.11, FL Studio 12.2, Studio One 3.1.1, Pro Tools 10.3.1.