Candidate Tidal Disruption Event AT2019fdr Coincident with a High-Energy Neutrino

Simeon Reusch; Robert Stein; Marek Kowalski; Sjoert Van Velzen; Anna Franckowiak; Cecilia Lunardini; Kohta Murase; Walter Winter; James C.A. Miller-Jones; Mansi M. Kasliwal; Marat Gilfanov; Simone Garrappa; Vaidehi S. Paliya; Tomás Ahumada; Shreya Anand; Cristina Barbarino; Eric C. Bellm; Valéry Brinnel; Sara Buson; S. Bradley Cenko; Michael W. Coughlin; Kishalay De; Richard Dekany; Sara Frederick; Avishay Gal-Yam; Suvi Gezari; Marcello Giroletti; Matthew J. Graham; Viraj Karambelkar; Shigeo S. Kimura; Albert K.H. Kong; Erik C. Kool; Russ R. Laher; Pavel Medvedev; Jannis Necker; Jakob Nordin; Daniel A. Perley; Mickael Rigault; Ben Rusholme; Steve Schulze; Tassilo Schweyer; Leo P. Singer; Jesper Sollerman; Nora Linn Strotjohann; Rashid Sunyaev; Jakob Van Santen; Richard Walters; B. Theodore Zhang; Erez Zimmerman

doi:10.1103/PhysRevLett.128.221101

Candidate Tidal Disruption Event AT2019fdr Coincident with a High-Energy Neutrino

Simeon Reusch^*, Robert Stein, Marek Kowalski^*, Sjoert Van Velzen, Anna Franckowiak, Cecilia Lunardini, Kohta Murase, Walter Winter, James C.A. Miller-Jones, Mansi M. Kasliwal, Marat Gilfanov, Simone Garrappa, Vaidehi S. Paliya, Tomás Ahumada, Shreya Anand, Cristina Barbarino, Eric C. Bellm, Valéry Brinnel, Sara Buson, S. Bradley CenkoMichael W. Coughlin, Kishalay De, Richard Dekany, Sara Frederick, Avishay Gal-Yam, Suvi Gezari, Marcello Giroletti, Matthew J. Graham, Viraj Karambelkar, Shigeo S. Kimura, Albert K.H. Kong, Erik C. Kool, Russ R. Laher, Pavel Medvedev, Jannis Necker, Jakob Nordin, Daniel A. Perley, Mickael Rigault, Ben Rusholme, Steve Schulze, Tassilo Schweyer, Leo P. Singer, Jesper Sollerman, Nora Linn Strotjohann, Rashid Sunyaev, Jakob Van Santen, Richard Walters, B. Theodore Zhang, Erez Zimmerman

^*Corresponding author for this work

Department of Particle Physics and Astrophysics

Research output: Contribution to journal › Article › peer-review

60 Citations (Scopus)

Abstract

The origins of the high-energy cosmic neutrino flux remain largely unknown. Recently, one high-energy neutrino was associated with a tidal disruption event (TDE). Here we present AT2019fdr, an exceptionally luminous TDE candidate, coincident with another high-energy neutrino. Our observations, including a bright dust echo and soft late-time x-ray emission, further support a TDE origin of this flare. The probability of finding two such bright events by chance is just 0.034%. We evaluate several models for neutrino production and show that AT2019fdr is capable of producing the observed high-energy neutrino, reinforcing the case for TDEs as neutrino sources.

Original language	English
Article number	221101
Journal	Physical review letters
Volume	128
Issue number	22
DOIs	https://doi.org/10.1103/PhysRevLett.128.221101
Publication status	Published - 3 Jun 2022

All Science Journal Classification (ASJC) codes

General Physics and Astronomy

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10.1103/PhysRevLett.128.221101

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Reusch, S., Stein, R., Kowalski, M., Van Velzen, S., Franckowiak, A., Lunardini, C., Murase, K., Winter, W., Miller-Jones, J. C. A., Kasliwal, M. M., Gilfanov, M., Garrappa, S., Paliya, V. S., Ahumada, T., Anand, S., Barbarino, C., Bellm, E. C., Brinnel, V., Buson, S., ... Zimmerman, E. (2022). Candidate Tidal Disruption Event AT2019fdr Coincident with a High-Energy Neutrino. Physical review letters, 128(22), Article 221101. https://doi.org/10.1103/PhysRevLett.128.221101

@article{2c1c0121c9814ac3a30ecdebbc29f174,

title = "Candidate Tidal Disruption Event AT2019fdr Coincident with a High-Energy Neutrino",

abstract = "The origins of the high-energy cosmic neutrino flux remain largely unknown. Recently, one high-energy neutrino was associated with a tidal disruption event (TDE). Here we present AT2019fdr, an exceptionally luminous TDE candidate, coincident with another high-energy neutrino. Our observations, including a bright dust echo and soft late-time x-ray emission, further support a TDE origin of this flare. The probability of finding two such bright events by chance is just 0.034%. We evaluate several models for neutrino production and show that AT2019fdr is capable of producing the observed high-energy neutrino, reinforcing the case for TDEs as neutrino sources.",

author = "Simeon Reusch and Robert Stein and Marek Kowalski and {Van Velzen}, Sjoert and Anna Franckowiak and Cecilia Lunardini and Kohta Murase and Walter Winter and Miller-Jones, {James C.A.} and Kasliwal, {Mansi M.} and Marat Gilfanov and Simone Garrappa and Paliya, {Vaidehi S.} and Tom{\'a}s Ahumada and Shreya Anand and Cristina Barbarino and Bellm, {Eric C.} and Val{\'e}ry Brinnel and Sara Buson and Cenko, {S. Bradley} and Coughlin, {Michael W.} and Kishalay De and Richard Dekany and Sara Frederick and Avishay Gal-Yam and Suvi Gezari and Marcello Giroletti and Graham, {Matthew J.} and Viraj Karambelkar and Kimura, {Shigeo S.} and Kong, {Albert K.H.} and Kool, {Erik C.} and Laher, {Russ R.} and Pavel Medvedev and Jannis Necker and Jakob Nordin and Perley, {Daniel A.} and Mickael Rigault and Ben Rusholme and Steve Schulze and Tassilo Schweyer and Singer, {Leo P.} and Jesper Sollerman and Strotjohann, {Nora Linn} and Rashid Sunyaev and {Van Santen}, Jakob and Richard Walters and Zhang, {B. Theodore} and Erez Zimmerman",

year = "2022",

month = jun,

day = "3",

doi = "10.1103/PhysRevLett.128.221101",

language = "English",

volume = "128",

journal = "Physical review letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "22",

}

Reusch, S, Stein, R, Kowalski, M, Van Velzen, S, Franckowiak, A, Lunardini, C, Murase, K, Winter, W, Miller-Jones, JCA, Kasliwal, MM, Gilfanov, M, Garrappa, S, Paliya, VS, Ahumada, T, Anand, S, Barbarino, C, Bellm, EC, Brinnel, V, Buson, S, Cenko, SB, Coughlin, MW, De, K, Dekany, R, Frederick, S, Gal-Yam, A, Gezari, S, Giroletti, M, Graham, MJ, Karambelkar, V, Kimura, SS, Kong, AKH, Kool, EC, Laher, RR, Medvedev, P, Necker, J, Nordin, J, Perley, DA, Rigault, M, Rusholme, B, Schulze, S, Schweyer, T, Singer, LP, Sollerman, J, Strotjohann, NL, Sunyaev, R, Van Santen, J, Walters, R, Zhang, BT & Zimmerman, E 2022, 'Candidate Tidal Disruption Event AT2019fdr Coincident with a High-Energy Neutrino', Physical review letters, vol. 128, no. 22, 221101. https://doi.org/10.1103/PhysRevLett.128.221101

TY - JOUR

T1 - Candidate Tidal Disruption Event AT2019fdr Coincident with a High-Energy Neutrino

AU - Reusch, Simeon

AU - Stein, Robert

AU - Kowalski, Marek

AU - Van Velzen, Sjoert

AU - Franckowiak, Anna

AU - Lunardini, Cecilia

AU - Murase, Kohta

AU - Winter, Walter

AU - Miller-Jones, James C.A.

AU - Kasliwal, Mansi M.

AU - Gilfanov, Marat

AU - Garrappa, Simone

AU - Paliya, Vaidehi S.

AU - Ahumada, Tomás

AU - Anand, Shreya

AU - Barbarino, Cristina

AU - Bellm, Eric C.

AU - Brinnel, Valéry

AU - Buson, Sara

AU - Cenko, S. Bradley

AU - Coughlin, Michael W.

AU - De, Kishalay

AU - Dekany, Richard

AU - Frederick, Sara

AU - Gal-Yam, Avishay

AU - Gezari, Suvi

AU - Giroletti, Marcello

AU - Graham, Matthew J.

AU - Karambelkar, Viraj

AU - Kimura, Shigeo S.

AU - Kong, Albert K.H.

AU - Kool, Erik C.

AU - Laher, Russ R.

AU - Medvedev, Pavel

AU - Necker, Jannis

AU - Nordin, Jakob

AU - Perley, Daniel A.

AU - Rigault, Mickael

AU - Rusholme, Ben

AU - Schulze, Steve

AU - Schweyer, Tassilo

AU - Singer, Leo P.

AU - Sollerman, Jesper

AU - Strotjohann, Nora Linn

AU - Sunyaev, Rashid

AU - Van Santen, Jakob

AU - Walters, Richard

AU - Zhang, B. Theodore

AU - Zimmerman, Erez

PY - 2022/6/3

Y1 - 2022/6/3

N2 - The origins of the high-energy cosmic neutrino flux remain largely unknown. Recently, one high-energy neutrino was associated with a tidal disruption event (TDE). Here we present AT2019fdr, an exceptionally luminous TDE candidate, coincident with another high-energy neutrino. Our observations, including a bright dust echo and soft late-time x-ray emission, further support a TDE origin of this flare. The probability of finding two such bright events by chance is just 0.034%. We evaluate several models for neutrino production and show that AT2019fdr is capable of producing the observed high-energy neutrino, reinforcing the case for TDEs as neutrino sources.

AB - The origins of the high-energy cosmic neutrino flux remain largely unknown. Recently, one high-energy neutrino was associated with a tidal disruption event (TDE). Here we present AT2019fdr, an exceptionally luminous TDE candidate, coincident with another high-energy neutrino. Our observations, including a bright dust echo and soft late-time x-ray emission, further support a TDE origin of this flare. The probability of finding two such bright events by chance is just 0.034%. We evaluate several models for neutrino production and show that AT2019fdr is capable of producing the observed high-energy neutrino, reinforcing the case for TDEs as neutrino sources.

UR - http://www.scopus.com/inward/record.url?scp=85131869176&partnerID=8YFLogxK

U2 - 10.1103/PhysRevLett.128.221101

DO - 10.1103/PhysRevLett.128.221101

M3 - Article

C2 - 35714251

AN - SCOPUS:85131869176

SN - 0031-9007

VL - 128

JO - Physical review letters

JF - Physical review letters

IS - 22

M1 - 221101

ER -

Candidate Tidal Disruption Event AT2019fdr Coincident with a High-Energy Neutrino

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