IceCube Group

IceCube Laboratory at the South Pole

The IceCube group at Harvard University is led by Prof. Carlos Argüelles-Delgado. Our main objective is to uncover new neutrino properties using high-energy atmospheric and astrophysical neutrinos. The neutrinos that we study have some of the highest energies ever observed and have traveled the longest distances from production to detection. This allows us to perform extreme tests of fundamental physics by using astrophysical neutrinos, which are very long interferometers. The main questions that our group tackles are the following:

  • What is the nature of neutrino masses?
  • What can we learn from the study of high-energy astrophysical neutrinos?
  • How do we use new technologies, such as machine learning or quantum computers, to increase the reach of our detectors?
  • How do we take neutrino telescopes to the next level? How should we build new ones?

To answer these questions, our group is engaged in every aspect of the experiment work and design, from hardware to high-level physics analyses.  More specifically, our physics data analyses work using more than ten years of data from the IceCube Neutrino Observatory, the largest neutrino telescope currently operating. We also work on machine learning applications for neutrino telescopes and the development of new Monte Carlo methods to improve the description of these detectors. We have a strong tradition of working closely with theorists to develop new ideas that end up as IceCube analyses. Finally, we are engaged in developing new devices for the upcoming IceCube Upgrade and developing new high-energy neutrino experiments such as TAMBO.

Project Areas

Particle Physics

We use high-energy neutrinos from the atmosphere and from astrophysical sources to test Standard Model predictions, make measurements, and search for new Beyond Standard Model (BSM) phenomena. We search for new particles, new forces, and new space-time symmetries. 

Data from IceCube on the search for light sterile neutrinos

Neutrino Astronomy

We develop new methods to search for neutrino sources and study their properties. We also use these cosmic baselengths to make conclusions about particle physics. 

Sources and oscillations

Hardware

We do a variety of hardware construction and testing for IceCube and broad outreach initiatives.

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Simulations and Software Development

We develop simulations and analysis software for IceCube and other neutrino telescopes. We are especially interested in open source neutrino event generator development. 

Simulation Stages

Companion Experiments

We are also involved in the development and analysis of other experiments that complement IceCube. 

  • TAMBO
  • KM3NeT
Neutrino experiments panorama

Outreach

We are involved in a variety of outreach projects aimed at secondary school students and the general public.

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Faculty

Postdoctoral Fellows

Graduate Students

Undergraduate Students

Laboratory for Particle Physics and Cosmology (LPPC), Harvard University.       18 Hammond Street, Cambridge, MA 02138, USA