Type text, add images, blackout confidential details, add comments, highlights and more.
02. Sign it in a few clicks
Draw your signature, type it, upload its image, or use your mobile device as a signature pad.
03. Share your form with others
Send it via email, link, or fax. You can also download it, export it or print it out.
How to quickly redact Latest Results on Direct Detection of Dark Matter WIMPs - IceCube online
Ease of Setup
DocHub User Ratings on G2
Ease of Use
DocHub User Ratings on G2
Dochub is the best editor for changing your forms online. Follow this straightforward guideline redact Latest Results on Direct Detection of Dark Matter WIMPs - IceCube in PDF format online for free:
Sign up and log in. Create a free account, set a secure password, and go through email verification to start managing your templates.
Add a document. Click on New Document and choose the file importing option: add Latest Results on Direct Detection of Dark Matter WIMPs - IceCube from your device, the cloud, or a secure URL.
Make changes to the template. Use the top and left-side panel tools to redact Latest Results on Direct Detection of Dark Matter WIMPs - IceCube. Insert and customize text, images, and fillable fields, whiteout unneeded details, highlight the important ones, and comment on your updates.
Get your documentation accomplished. Send the form to other parties via email, create a link for quicker document sharing, export the template to the cloud, or save it on your device in the current version or with Audit Trail included.
Try all the benefits of our editor today!
Fill out Latest Results on Direct Detection of Dark Matter WIMPs - IceCube online It's free
Researchers use large, sensitive detectors located deep underground to directly search for the dark matter particles that may continually pass through the Earth. Researchers can also search for dark matter indirectly through specific signatures in cosmic rays and gamma rays.
What is the best evidence for dark matter?
One particular galaxy cluster, known as the Bullet Cluster, provides some of the best evidence we have for the existence of dark matter. This cluster is made up of two smaller clusters that collided sometime in the past.
What is detected by the IceCube experiment in Antarctica?
IceCube detects light emitted by charged particles that are produced when a single neutrino crashes into a proton or neutron inside an atom. The resulting nuclear reaction produces secondary particles traveling at high speeds (faster than light in the ice!) that give off a blue light called Cherenkov radiation.
How many neutrinos has IceCube detected?
Neutrino Physics. IceCube has recorded an unusually large set of neutrinos. From over ten years data, we have accumulated about 700,000 between 100 GeV and 1 PeV and 200,000 between 10 GeV and 100 GeV. Both datasets have outstanding purity, at more than 99% with respect to downgoing cosmic ray muons.
Can an IceCube detect dark matter?
We compare our model projections with the most current constraints and show that the IceCube detector can detect CR-boosted dark matter especially with masses below when scattering with electrons and in the nucleon scattering case.
One of the only experiments to detect axions as dark matter is the Axion Dark Matter Experiment (ADMX). Located at the University of Washington, ADMX uses a resonant microwave cavity in a strong magnetic field to convert dark matter into microwave photons by means of the Primakoff effect.
What is the direct detection of dark matter experiment?
Direct detection of dark matter is based upon the premise that since it is known that dark matter exists in some form, Earth must intercept some as it carves out a path through the universe. Direct detection experiments attempt to create highly sensitive systems capable of detecting these rare and weak events.
What does IceCube detect?
IceCube detects high-energy neutrinos using the Cherenkov light produced by relativistic charged particles that result from the interaction of these neutrinos with the atomic nuclei of Antarctic ice.
Related links
The users manual, version 5.0 | MicroMegas - LAPTh - CNRS
by D Barducci 2019 First developed to compute the relic density of dark matter, the code also computes the rates for dark matter direct and indirect detection. micrOMEGAs.
2023 Cited by 2 Recent IceCube analyses derived one of the best bounds on the dark matter lifetime on the TeV-PeV scale, by looking for neutrinos from Galactic
This site uses cookies to enhance site navigation and personalize your experience.
By using this site you agree to our use of cookies as described in our Privacy Notice.
You can modify your selections by visiting our Cookie and Advertising Notice.... Read more...Read less