Measurement of Atmospheric Neutrino Oscillations with Very Large Volume Neutrino Telescopes

<div>Distribution of events as a function of reconstructed <svg height="11.4781pt" id="M205" style="vertical-align:-2.18977pt" version="1.1" viewbox="-0.0498162 -9.28833 21.1472 11.4781" width="21.1472pt" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink"><g transform="matrix(.013,0,0,-0.013,0,0)"><path d="M567 167L534 181C505 122 482 94 454 70C428 46 385 42 330 42C288 42 248 44 235 55C216 70 213 91 220 130L295 528C310 609 314 611 401 618L409 650H140L131 618C222 611 224 609 209 528L133 126C118 47 108 41 25 33L18 0H497C514 33 554 126 567 167Z" id="g50-77"></path><glyph.data ascent="3443" descent="-2856" horiz-adv-x="579" vert-adv-y="579"></glyph.data></g><g transform="matrix(.013,0,0,-0.013,7.289,0)"><path d="M381 704H317L48 -163H112L381 704Z" id="g50-48"></path><glyph.data ascent="3443" descent="-2856" horiz-adv-x="429" vert-adv-y="429"></glyph.data></g><g transform="matrix(.013,0,0,-0.013,12.871,0)"><path d="M615 650H141L132 618C223 612 227 607 212 526L136 123C122 42 112 38 27 32L18 0H522C539 33 580 135 592 166L558 179C536 139 512 100 486 75C454 48 420 41 345 41C287 41 252 42 237 55C221 68 220 100 231 158L261 316H357C455 316 455 309 455 235H489L529 437H494C468 366 460 360 369 360H269L305 565C315 609 316 611 357 611H450C525 611 535 599 548 578C559 556 561 526 560 482L595 486L615 650Z" id="g50-70"></path><glyph.data ascent="3443" descent="-2856" horiz-adv-x="639" vert-adv-y="639"></glyph.data></g></svg> of IceCube’s IC86-B analysis. Data are compared to the best fit and expectation with no oscillations (a) and the ratio of data and best fit to the expectation without oscillations is also shown (b). Bands indicate estimated systematic uncertainties. From [<a href="/journals/ahep/2015/271968/#B9">9</a>].</div>

Advances in High Energy Physics

fig15

Figure 15

Figure 15: Measurement of Atmospheric Neutrino Oscillations with Very Large Volume Neutrino Telescopes 