المؤلفون: Eckner, Christopher, Calore, Francesca, Erkal, Denis, Lilleengen, Sophia, Petersen, Michael S.

المساهمون: Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), ANR-19-CE31-0017,SEGAL,Evolution séculaire des galaxies(2019), ANR-19-CE31-0005,GECO,Émissions Galactiques de haute énergie des objets compacts(2019)

المصدر: ISSN: 0035-8711.

مصطلحات موضوعية: dark matter: halo, scale: electroweak interaction, gamma ray: emission, cross section: annihilation, dark matter: annihilation, galaxy, cloud, satellite, density, GLAST, numerical calculations, deformation, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]

العلاقة: info:eu-repo/semantics/altIdentifier/arxiv/2208.03312; hal-03763002; https://hal.science/hal-03763002Test; https://hal.science/hal-03763002/documentTest; https://hal.science/hal-03763002/file/stac3340.pdfTest; ARXIV: 2208.03312; INSPIRE: 2132754

الإتاحة: https://doi.org/10.1093/mnras/stac3340Test
https://hal.science/hal-03763002Test
https://hal.science/hal-03763002/documentTest
https://hal.science/hal-03763002/file/stac3340.pdfTest

المؤلفون: Eckner, Christopher, Calore, Francesca, Erkal, Denis, Lilleengen, Sophia, Petersen, Michael S.

المساهمون: Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), ANR-19-CE31-0017,SEGAL,Evolution séculaire des galaxies(2019), ANR-19-CE31-0005,GECO,Émissions Galactiques de haute énergie des objets compacts(2019)

المصدر: ISSN: 0035-8711.

مصطلحات موضوعية: dark matter: halo, scale: electroweak interaction, gamma ray: emission, cross section: annihilation, dark matter: annihilation, galaxy, cloud, satellite, density, GLAST, numerical calculations, deformation, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]

العلاقة: info:eu-repo/semantics/altIdentifier/arxiv/2208.03312; hal-03763002; https://hal.science/hal-03763002Test; https://hal.science/hal-03763002/documentTest; https://hal.science/hal-03763002/file/stac3340.pdfTest; ARXIV: 2208.03312; INSPIRE: 2132754

الإتاحة: https://doi.org/10.1093/mnras/stac3340Test
https://hal.science/hal-03763002Test
https://hal.science/hal-03763002/documentTest
https://hal.science/hal-03763002/file/stac3340.pdfTest

المؤلفون: Eckner, Christopher, Calore, Francesca, Erkal, Denis, Lilleengen, Sophia, Petersen, Michael S.

المساهمون: Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), ANR-19-CE31-0017,SEGAL,Evolution séculaire des galaxies(2019), ANR-19-CE31-0005,GECO,Émissions Galactiques de haute énergie des objets compacts(2019)

المصدر: ISSN: 0035-8711.

مصطلحات موضوعية: dark matter: halo, scale: electroweak interaction, gamma ray: emission, cross section: annihilation, dark matter: annihilation, galaxy, cloud, satellite, density, GLAST, numerical calculations, deformation, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]

العلاقة: info:eu-repo/semantics/altIdentifier/arxiv/2208.03312; hal-03763002; https://hal.science/hal-03763002Test; https://hal.science/hal-03763002/documentTest; https://hal.science/hal-03763002/file/stac3340.pdfTest; ARXIV: 2208.03312; INSPIRE: 2132754

الإتاحة: https://doi.org/10.1093/mnras/stac3340Test
https://hal.science/hal-03763002Test
https://hal.science/hal-03763002/documentTest
https://hal.science/hal-03763002/file/stac3340.pdfTest

المؤلفون: Eckner, Christopher, Calore, Francesca, Erkal, Denis, Lilleengen, Sophia, Petersen, Michael S.

المساهمون: Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), ANR-19-CE31-0017,SEGAL,Evolution séculaire des galaxies(2019), ANR-19-CE31-0005,GECO,Émissions Galactiques de haute énergie des objets compacts(2019)

المصدر: ISSN: 0035-8711.

مصطلحات موضوعية: dark matter: halo, scale: electroweak interaction, gamma ray: emission, cross section: annihilation, dark matter: annihilation, galaxy, cloud, satellite, density, GLAST, numerical calculations, deformation, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]

العلاقة: info:eu-repo/semantics/altIdentifier/arxiv/2208.03312; hal-03763002; https://hal.science/hal-03763002Test; https://hal.science/hal-03763002/documentTest; https://hal.science/hal-03763002/file/stac3340.pdfTest; ARXIV: 2208.03312; INSPIRE: 2132754

الإتاحة: https://doi.org/10.1093/mnras/stac3340Test
https://hal.science/hal-03763002Test
https://hal.science/hal-03763002/documentTest
https://hal.science/hal-03763002/file/stac3340.pdfTest

المؤلفون: Eckner, Christopher, Calore, Francesca, Erkal, Denis, Lilleengen, Sophia, Petersen, Michael S.

المساهمون: Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)

المصدر: Mon.Not.Roy.Astron.Soc. ; https://hal.science/hal-03763002Test ; Mon.Not.Roy.Astron.Soc., 2023, 518 (3), pp.4138-4158. ⟨10.1093/mnras/stac3340⟩

مصطلحات موضوعية: dark matter: halo, scale: electroweak interaction, gamma ray: emission, cross section: annihilation, dark matter: annihilation, galaxy, cloud, satellite, density, GLAST, numerical calculations, deformation, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]

العلاقة: info:eu-repo/semantics/altIdentifier/arxiv/2208.03312; hal-03763002; https://hal.science/hal-03763002Test; ARXIV: 2208.03312; INSPIRE: 2132754

الإتاحة: https://doi.org/10.1093/mnras/stac3340Test
https://hal.science/hal-03763002Test