Neutrinos in Cosmology and Astrophysics

6 Mar 2024, 09:00 → 8 Mar 2024, 17:00 US/Pacific

Auditorium (TRIUMF)

Neutrinos play a crucial role in cosmology and astrophysics. They may also connect to the mysteries of dark matter and the matter-antimatter asymmetry. With many exciting new observations, measurements, and calculations expected in the coming years, it is good time to investigate what we might learn and the potential implications for fundamental physics. This workshop will bring together a diverse range of theorists and experimentalists to new directions in neutrino physics and their connections with cosmology and astrophysics.

While most of the workshop will be in-person, a remote connection will be offered as well. Please note that in-person attendance will be limited by the size of the venue. If you would like to attend at TRIUMF, please register by February 16, 2024. 

Wednesday, 6 March

1 Welcome to TRIUMF!

Speakers: Carlos Henrique de Lima (TRIUMF), David McKeen (TRIUMF), David Morrissey (TRIUMF), Douglas Tuckler (TRIUMF and Simon Fraser University), Gopolang Mohlabeng (Simon Fraser University and TRIUMF), Lilianna Hariasz (Queen's University), Michael Shamma (TRIUMF), Nicole Vassh (TRIUMF), Ricky Mizuta (TRIUMF / University of British Columbia), Tsung-Han Yeh (TRIUMF)

2 Neutrino Mixing from Modular Flavor Symmetries

Speaker: Mu-Chun Chen (UC Irvine)

2024TRIUMF_MCChen.pdf

3 Neutrinos: their origin and their role in the matter-antimatter asymmetry

Speaker: Arnab Dasgupta (U Pittsburgh)

Dasgupta.pdf

4 Cosmology of Dirac Neutrino Mass Models

Speaker: Michael Shamma (TRIUMF)

Shamma.pdf

14:30 Tea and Cookies

5 A low-scale neutrino mass model and energy-dependent oscillation parameters

Speaker: Pedro Machado (Fermilab)

Machado.pdf

6 Discovering (A) Source of Neutrino Masses at the LHC

Speaker: Seyda Ipek

Ipek.pdf

7 Old Data, New Forensics: The First Second of SN 1987A Neutrino Emission

Speaker: Shirley Li (UC Irvine)

Li.pdf

8 Open Discussion

Thursday, 7 March

9 Relic neutrinos from collapsars and neutron star mergers

In highly dense matter scenarios, such as in Supernova, collapsars, and neutron star mergers, neutrinos decouple from matter much earlier and deeper than photons. Their detection in neutrino observatories would allow us to gain valuable insight into the interior, structure, and evolution of these astrophysical environments. While much can be learned from the neutrinos emitted by a single explosion, the rarity of these events combined with neutrinos' weakly interacting nature pose challenges for their detection. Relic neutrinos, emitted since the first Supernovae and mergers occurred in the universe, provide a continuous background flux that offers an additional avenue for the study of matter under strong gravity. In this talk, I shall discuss the diffuse neutrino background from collapsars and neutron star mergers, and the prospects of learning about the equation of state of nuclear matter from its possible detection.

Speaker: Liliana Caballero (U Guelph)

Caballero.pdf

10 Neutrinos, Collapsars, Neutron Star Mergers, and You: How neutrinos impact heavy element formation in the universe, and the resulting electromagnetic counterpart

Speaker: Jonah Miller (Los Alamos)

Miller.pdf

10:30 Tea and Cookies

11 Probing turbulence in core-collapse supernovae in the upcoming neutrino detectors

Speaker: Mainak Mukhopadhyay (Penn State U)

Mainak.pdf

12 Presupernova Neutrinos: Realistic Emissivities and Detection Possibilities

Speaker: Kelly Patton (Trinity College)

Patton.pdf

13 P-ONE Neutrino Observatory

Speaker: Matthias Danninger (Simon Fraser University)

Danninger.pdf

12:30 Lunch

14 TRIUMF Colloquium - Core-collapse supernovae as probes of (not only) non-standard neutrino physics

Core-collapse supernovae are one of the most complex phenomena in the Universe. Not only are they one of the production sites of the heavy elements that enable the existence of life, but their cores are also one of the densest environments we can probe, albeit indirectly. Core-collapse supernovae are also among the most spectacular and efficient neutrino factories. Detecting these neutrinos can allow us to probe physics in extreme conditions inaccessible on Earth. In this talk, I will discuss how we can prepare for the next nearby supernova neutrino detection to extract as much information as possible from the neutrino signal. I will also talk about how observing neutrinos from all the past collapses in our Universe – the diffuse supernova neutrino background - can help us better understand the supernova population and may provide hints about physics beyond the Standard Model.

Speaker: Anna Suliga (UC Berkely / N3AS)

Suliga.pdf

15 Entaglement of Astrophysical Neutrinos

Speaker: Baha Balantekin (U Wisconsin)

Balantekin.pdf

16 Open Discussion

18:00 Workshop Dinner

Lebanese restaurant with vegetarian and vegan options.

3116 W Broadway
604-336-1797

https://www.nuba.ca/kitsilano

Friday, 8 March

17 Neutrinos vs. Dark Matter

Speaker: Kevin Kelly (Texas A&M)

Kelly.pdf

18 Probes of Neutrinophilc Dark Matter

Speaker: Douglas Tuckler (TRIUMF and Simon Fraser University)

DTuckler_NeutrinophilicDM.pdf

10:30 Tea and Cookies

19 Origins of (neutrino-ish) Dark Matter in the Matter Power Spectrum

Speaker: Yue Zhang (Carleton U)

Zhang.pdf

20 The flavour of high-energy neutrinos

Speaker: Aaron Vincent (Queen's U)

Vincent.pdf

21 Neutrinos as standard and nonstandard dark radiation and dark matter

Speaker: Kevork Abazajian (UC Irvine)

Abazajian 2024 TRIUMF.pdf

12:30 Lunch