Semantic Scholar Open Access 2024 11 sitasi

Constraints on axion-like particles with the Perseus Galaxy Cluster with MAGIC

M. Abe S. Abe J. Abhir V. Acciari I. Agudo +372 lainnya

Abstrak

Axion-like particles (ALPs) are pseudo-Nambu-Goldstone bosons that emerge in various theories beyond the standard model. These particles can interact with high-energy photons in external magnetic fields, influencing the observed gamma-ray spectrum. This study analyzes 41.3 hrs of observational data from the Perseus Galaxy Cluster collected with the MAGIC telescopes. We focused on the spectra the radio galaxy in the center of the cluster: NGC 1275. By modeling the magnetic field surrounding this target, we searched for spectral indications of ALP presence. Despite finding no statistical evidence of ALP signatures, we were able to exclude ALP models in the sub-micro electronvolt range. Our analysis improved upon previous work by calculating the full likelihood and statistical coverage for all considered models across the parameter space. Consequently, we achieved the most stringent limits to date for ALP masses around 50 neV, with cross sections down to $g_{a\gamma} = 3 \times 10^{-12}$ GeV$^{-1}$.

Topik & Kata Kunci

Penulis (377)

M

M. Abe

S

S. Abe

J

J. Abhir

V

V. Acciari

I

I. Agudo

T

T. Aniello

S

S. Ansoldi

L

L. A. Antonelli

A

A. Engels

C

C. Arcaro

M

M. Artero

K

K. Asano

D

D. Baack

A

A. Babi'c

A

A. Baquero

U

U. D. Almeida

J

J. Barrio

I

I. Batkovi'c

J

J. Baxter

J

J. B. Gonz'alez

W

W. Bednarek

E

E. Bernardini

J

J. Bernete

A

A. Berti

J

J. Besenrieder

C

C. Bigongiari

A

A. Biland

O

O. Blanch

G

G. Bonnoli

v

vZ. Bovsnjak

I

I. Burelli

G

G. Busetto

A

A. Campoy-Ordaz

A

A. Carosi

R

R. Carosi

M

M. Carretero-Castrillo

A

A. Castro-Tirado

G

G. Ceribella

Y

Y. Chai

A

A. Cifuentes

S

S. Cikota

E

E. Colombo

J

J. Contreras

J

J. Cortina

S

S. Covino

G

G. D'Amico

V

V. D’Elia

P

P. D. Vela

F

F. Dazzi

A

A. D. Angelis

B

B. Lotto

A

A. Popolo

J

J. Delgado

C

C. Mendez

D

D. Depaoli

F

F. Pierro

L

L. Venere

A

A. Donini

D

D. Dorner

M

M. Doro

D

D. Elsaesser

G

G. Emery

J

J. Escudero

L

L. Fariña

A

A. Fattorini

L

L. Foffano

L

L. Font

S

S. Fukami

Y

Y. Fukazawa

R

R. L'opez

M

M. Garczarczyk

S

S. Gasparyan

M

M. Gaug

J

J. Paiva

N

N. Giglietto

F

F. Giordano

P

P. Gliwny

N

N. Godinovi'c

R

R. Grau

D

D. Green

J

J. Green

D

D. Hadasch

A

A. Hahn

T

T. Hassan

L

L. Heckmann

J

J. Herrera

D

D. Hrupec

M

M. Hutten

R

R. Imazawa

T

T. Inada

R

R. Iotov

K

K. Ishio

I

I. Mart'inez

J

J. Jormanainen

D

D. Kerszberg

G

G. Kluge

Y

Y. Kobayashi

P

P. M. Kouch

H

H. Kubo

J

J. Kushida

M

M. L'ainez

A

A. Lamastra

F

F. Leone

E

E. Lindfors

L

L. Linhoff

S

S. Lombardi

F

F. Longo

R

R. L'opez-Coto

M

M. L'opez-Moya

A

A. L'opez-Oramas

S

S. Loporchio

A

A. Lorini

B

B. Fraga

P

P. Majumdar

M

M. Makariev

G

G. Maneva

N

N. Mang

M

M. Manganaro

S

S. Mangano

K

K. Mannheim

M

M. Mariotti

M

M. Mart'inez

M

M. Mart'inez-Chicharro

A

A. Mas-Aguilar

D

D. Mazin

S

S. Menchiari

S

S. Mender

D

D. Miceli

T

T. Miener

J

J. Miranda

R

R. Mirzoyan

M

M. Gonz'alez

E

E. Molina

H

H. A. Mondal

A

A. Moralejo

D

D. Morcuende

T

T. Nakamori

C

C. Nanci

L

L. Nava

V

V. Neustroev

L

L. Nickel

M

M. Rosillo

C

C. Nigro

L

L. Nikoli'c

K

K. Nilsson

K

K. Nishijima

T

T. Ekoume

K

K. Noda

S

S. Nozaki

Y

Y. Ohtani

A

A. Okumura

J

J. Otero-Santos

S

S. Paiano

M

M. Palatiello

D

D. Paneque

R

R. Paoletti

J

J. Paredes

D

D. Pavlovi'c

M

M. Persic

M

M. Pihet

G

G. Pirola

F

F. Podobnik

P

P. Moroni

E

E. Prandini

G

G. Principe

C

C. Priyadarshi

W

W. Rhode

M

M. Rib'o

J

J. Rico

C

C. Righi

N

N. Sahakyan

T

T. Saito

K

K. Satalecka

F

F. Saturni

B

B. Schleicher

K

K. Schmidt

F

F. Schmuckermaier

J

J. L. Schubert

T

T. Schweizer

A

A. Sciaccaluga

J

J. Sitarek

V

V. Sliusar

D

D. Sobczynska

A

A. Spolon

A

A. Stamerra

J

J. Strivskovi'c

D

D. Strom

M

M. Strzys

Y

Y. Suda

S

S. Suutarinen

H

H. Tajima

M

M. Takahashi

R

R. Takeishi

F

F. Tavecchio

P

P. Temnikov

K

K. Terauchi

T

T. Terzi'c

M

M. Teshima

L

L. Tosti

S

S. Truzzi

A

A. Tutone

S

S. Ubach

J

J. Scherpenberg

M

M. Acosta

S

S. Ventura

V

V. Verguilov

I

I. Viale

C

C. Vigorito

V

V. Vitale

I

I. Vovk

R

R. Walter

M

M. Will

T

T. Yamamoto

J

J. I. F. C. Research

T

T. U. O. Tokyo

K

Kashiwa

2

277-8582 Chiba

J

Japan.

E

E. Zurich

C

CH-8093 Zurich

S

Switzerland.

I

Instituto de Astrof'isica de Canarias

D

D. Astrof'isica

U

U. L. Laguna

E

E-38200

L

L. Laguna

T

Tenerife

S

Spain.

I

Instituto de Astrof'isica de Andaluc'ia-CSIC

G

Glorieta de la Astronom'ia sn

1

18008

G

Granada

N

National Centre for Radio Astrophysics

I

I-00136 Rome

I

Italy

U

U. Udine

I

I. Trieste

I

I. Udine

M

M. F. Physik

D

D. Garching

G

Germany

U

U. Padova

I

Infn

I

I-35131 Padova

I

Institut de F'isica d'Altes Energies

T

T. Z. F. O. Science

T

Technology

E

E-08193 Bellaterra

T

Technische Universitat Dortmund

D

D. Dortmund

C

C. Zagreb

F

Faculty of Electrical Engineering

C

Computing

1

10000 Zagreb

C

Croatia.

I

I. Institute

E

E. Department

U

U. Madrid

E

E. Madrid

C

Centro Brasileiro de Pesquisas F'isicas

2

22290-180 Urca

R

R. Janeiro

B

Brazil

U

U. Lodz

F

F. O. Physics

A

Applied Informatics

D

D. O. Astrophysics

9

9. Lodz

P

Poland

C

Centro de Investigaciones Energ'eticas

M

Medioambientales y Tecnol'ogicas

D

Departament de F'isica

C

CERES-IEEC

U

U. Barcelona

U

U. Pisa

I

I. Pisa

I

I. Pisa

U

U. Barcelona

I

Iccub

I

IEEC-UB

E

E. Barcelona

D

Department for Physics

U

Universityof Bergen

N

Norway.

I

I. Catania

D

D. Astronomia

U

U. Catania

I

I. Catania

I

I. Torino

U

U. Torino

I

I. Torino

I

I. Bari

D

D. Bari

I

I. Bari

U

U. Wurzburg

D

D-97074 Wurzburg

U

U. Geneva

1

16 Chemind'Ecogia

C

CH-1290 Versoix

J

Japanese Magic Group Physics Program

G

Graduate School of Science

E

Engineering

H

H. University

7

739-8526 Hiroshima

D

D. Elektronen-Synchrotron

D

D. Zeuthen

A

Armenian Magic Group ICRANet-Armenia

0

0019 Yerevan

A

Armenia

C

C. Split

M

M. Engineering

N

Naval Architecture

2

21000 Split

C

Croatia Croatian Magic Group Josip Juraj Strossmayer Unive Osijek

D

D. Physics

3

31000 Osijek

F

Finnish Magic Consortium Finnish Centre of Astronomy with Eso

A

Astronomy

U

U. Turku

F

F. Turku

F

Finland.

J

J. D. O. Physics

T

T. University

H

Hiratsuka

2

259-1292 Kanagawa

U

U. Siena

I

I-53100 Siena

S

S. S. I. O. Physics

A

A. C. O. L. P. Institute

K

Kolkata 700064

W

West Bengal

I

India.

I

Inst. for Nucl. Research

N

Nucl. Energy

B

B. A. O. Sciences

B

BG-1784 Sofia

B

Bulgaria.

C

C. Rijeka

5

51000 Rijeka

Y

Yamagata University

Y

Yamagata 990-8560

F

Finnish Magic Group Space Physics

A

A. Unit

U

U. Oulu

F

F. Oulu

J

Japanese Magic Group Chiba University

I

Icehap

2

277-8582 Chiba

J

J. I. F. C. Research

K

Kobayashi-Maskawa Institute for the Origin of Particles

t

the Universe

N

N. University

4

464-6801 Nagoya

K

Kyoto University

6

606-8502 Kyoto

I

I. Perugia

I

I. Perugia

I

I. Vergata

I

I. Roma

K

K. University

K

Kobe

H

Hyogo 658-8501

A

A. M. C. F. Astrophysics

R

Romé

a

also at Port d'Informaci'o Cient'ifica

a

also at Institute for Astro-

P

P. Physics

U

U. Innsbruck

A

A. Innsbruck

M

M Austria

A

A. D. O. Physics

U

U. Oslo

A

A. N. D. D. Fisica

U

U. Trieste

I

I. Trieste

D

D-80805 Munchen

a

also at Inaf Padova

Format Sitasi

Abe, M., Abe, S., Abhir, J., Acciari, V., Agudo, I., Aniello, T. et al. (2024). Constraints on axion-like particles with the Perseus Galaxy Cluster with MAGIC. https://doi.org/10.1016/j.dark.2024.101425

Akses Cepat

Lihat di Sumber doi.org/10.1016/j.dark.2024.101425
Informasi Jurnal
Tahun Terbit
2024
Bahasa
en
Total Sitasi
11×
Sumber Database
Semantic Scholar
DOI
10.1016/j.dark.2024.101425
Akses
Open Access ✓