Brazilian Community Report on Dark Matter
This white paper summarizes the activities of the Brazilian community concerning dark matter physics and highlights the importance of financial support to Brazilian groups that are deeply involved in experimental endeavours. The flagships of the Brazilian dark matter program are the Cherenkov Telesc...
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| creator | Abdalla, E Albuquerque, I. F. M Alves, A Barosi, L Bazetto, M. C. Q Batista, R. C Bernardes, C. A Bonifazi, C Borges, H. A Brito, F. A Caramês, T. R. P Casarini, L Cogollo, D Dias, A. G Esmaili, A Ferreira, M. M da Silveira, G. Gil Guzzo, M. M Hadjimichef, D de Holanda, P. C Kemp, E Lessa, A Lichtenstein, G Machado, A. A Makler, M Marra, V Matheus, R. D Mercadante, P. G de Melo, T. B Nishi, C Nepomuceno, A Novaes, S. F Pimentel, V. L Pinheiro, P. R. D Pires, C. A Queiroz, A. R Queiroz, F. S ~Rangel, M. ~S Rodrigues, D. C Rodrigues, J. G de Souza, V da Silva, P. S. Rodrigues Siqueira, C Segreto, E Sanchez-Vega, B. L Rosenfeld, R Santos, J. R. L Santos, A. C. O Silva, R Sokolowska, D Teles, P. R Tomei, T. R. F. P Valdiviesso, G. A Vasconcelos, P Viana, A |
| description | This white paper summarizes the activities of the Brazilian community
concerning dark matter physics and highlights the importance of financial
support to Brazilian groups that are deeply involved in experimental
endeavours. The flagships of the Brazilian dark matter program are the
Cherenkov Telescope Array, DARKSIDE, SBN and LHC experiments, but we emphasize
that smaller experiments such as DAMIC and CONNIE constitute important probes
to dark sectors as well and should receive special attention. Small
experimental projects showing the potential to probe new regions of parameter
space of dark matter models are encouraged. On the theoretical and
phenomenological side, some groups are devoted to astrophysical aspects such as
the dark matter density profile while others explore the signature of dark
matter models at colliders, direct and indirect detection experiments. In
summary, the Brazilian dark matter community that was born not long ago has
grown tremendously in the past years and now plays an important role in the
hunt for a dark matter particle. |
| doi_str_mv | 10.48550/arxiv.1912.10076 |
| format | Article |
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concerning dark matter physics and highlights the importance of financial
support to Brazilian groups that are deeply involved in experimental
endeavours. The flagships of the Brazilian dark matter program are the
Cherenkov Telescope Array, DARKSIDE, SBN and LHC experiments, but we emphasize
that smaller experiments such as DAMIC and CONNIE constitute important probes
to dark sectors as well and should receive special attention. Small
experimental projects showing the potential to probe new regions of parameter
space of dark matter models are encouraged. On the theoretical and
phenomenological side, some groups are devoted to astrophysical aspects such as
the dark matter density profile while others explore the signature of dark
matter models at colliders, direct and indirect detection experiments. In
summary, the Brazilian dark matter community that was born not long ago has
grown tremendously in the past years and now plays an important role in the
hunt for a dark matter particle.</description><identifier>DOI: 10.48550/arxiv.1912.10076</identifier><language>eng</language><subject>Physics - Cosmology and Nongalactic Astrophysics ; Physics - High Energy Astrophysical Phenomena ; Physics - High Energy Physics - Phenomenology</subject><creationdate>2019-12</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,781,886</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/1912.10076$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.1912.10076$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Abdalla, E</creatorcontrib><creatorcontrib>Albuquerque, I. F. M</creatorcontrib><creatorcontrib>Alves, A</creatorcontrib><creatorcontrib>Barosi, L</creatorcontrib><creatorcontrib>Bazetto, M. C. Q</creatorcontrib><creatorcontrib>Batista, R. C</creatorcontrib><creatorcontrib>Bernardes, C. A</creatorcontrib><creatorcontrib>Bonifazi, C</creatorcontrib><creatorcontrib>Borges, H. A</creatorcontrib><creatorcontrib>Brito, F. A</creatorcontrib><creatorcontrib>Caramês, T. R. P</creatorcontrib><creatorcontrib>Casarini, L</creatorcontrib><creatorcontrib>Cogollo, D</creatorcontrib><creatorcontrib>Dias, A. G</creatorcontrib><creatorcontrib>Esmaili, A</creatorcontrib><creatorcontrib>Ferreira, M. M</creatorcontrib><creatorcontrib>da Silveira, G. Gil</creatorcontrib><creatorcontrib>Guzzo, M. M</creatorcontrib><creatorcontrib>Hadjimichef, D</creatorcontrib><creatorcontrib>de Holanda, P. C</creatorcontrib><creatorcontrib>Kemp, E</creatorcontrib><creatorcontrib>Lessa, A</creatorcontrib><creatorcontrib>Lichtenstein, G</creatorcontrib><creatorcontrib>Machado, A. A</creatorcontrib><creatorcontrib>Makler, M</creatorcontrib><creatorcontrib>Marra, V</creatorcontrib><creatorcontrib>Matheus, R. D</creatorcontrib><creatorcontrib>Mercadante, P. G</creatorcontrib><creatorcontrib>de Melo, T. B</creatorcontrib><creatorcontrib>Nishi, C</creatorcontrib><creatorcontrib>Nepomuceno, A</creatorcontrib><creatorcontrib>Novaes, S. F</creatorcontrib><creatorcontrib>Pimentel, V. L</creatorcontrib><creatorcontrib>Pinheiro, P. R. D</creatorcontrib><creatorcontrib>Pires, C. A</creatorcontrib><creatorcontrib>Queiroz, A. R</creatorcontrib><creatorcontrib>Queiroz, F. S</creatorcontrib><creatorcontrib>~Rangel, M. ~S</creatorcontrib><creatorcontrib>Rodrigues, D. C</creatorcontrib><creatorcontrib>Rodrigues, J. G</creatorcontrib><creatorcontrib>de Souza, V</creatorcontrib><creatorcontrib>da Silva, P. S. Rodrigues</creatorcontrib><creatorcontrib>Siqueira, C</creatorcontrib><creatorcontrib>Segreto, E</creatorcontrib><creatorcontrib>Sanchez-Vega, B. L</creatorcontrib><creatorcontrib>Rosenfeld, R</creatorcontrib><creatorcontrib>Santos, J. R. L</creatorcontrib><creatorcontrib>Santos, A. C. O</creatorcontrib><creatorcontrib>Silva, R</creatorcontrib><creatorcontrib>Sokolowska, D</creatorcontrib><creatorcontrib>Teles, P. R</creatorcontrib><creatorcontrib>Tomei, T. R. F. P</creatorcontrib><creatorcontrib>Valdiviesso, G. A</creatorcontrib><creatorcontrib>Vasconcelos, P</creatorcontrib><creatorcontrib>Viana, A</creatorcontrib><title>Brazilian Community Report on Dark Matter</title><description>This white paper summarizes the activities of the Brazilian community
concerning dark matter physics and highlights the importance of financial
support to Brazilian groups that are deeply involved in experimental
endeavours. The flagships of the Brazilian dark matter program are the
Cherenkov Telescope Array, DARKSIDE, SBN and LHC experiments, but we emphasize
that smaller experiments such as DAMIC and CONNIE constitute important probes
to dark sectors as well and should receive special attention. Small
experimental projects showing the potential to probe new regions of parameter
space of dark matter models are encouraged. On the theoretical and
phenomenological side, some groups are devoted to astrophysical aspects such as
the dark matter density profile while others explore the signature of dark
matter models at colliders, direct and indirect detection experiments. In
summary, the Brazilian dark matter community that was born not long ago has
grown tremendously in the past years and now plays an important role in the
hunt for a dark matter particle.</description><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - High Energy Physics - Phenomenology</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotzjsLwjAYheEsDlL9AU5mdWjNZ2yajFqvoAjiXj6bBIK9SKyi_nqv01leDg8hPWDRWMYxG6K_u1sECkYRMJaINhlMPT5d4bCiaV2W18o1D7o359o3tK7oDP2JbrFpjO-QlsXiYrr_DchhMT-kq3CzW67TySZEkYgQubQorAVAIa0yOjcmZvoIudVaKQE4kkrJnEvJ34wE43eokQmQKueM8YD0f7dfa3b2rkT_yD7m7GvmLzRDOzI</recordid><startdate>20191220</startdate><enddate>20191220</enddate><creator>Abdalla, E</creator><creator>Albuquerque, I. F. M</creator><creator>Alves, A</creator><creator>Barosi, L</creator><creator>Bazetto, M. C. Q</creator><creator>Batista, R. C</creator><creator>Bernardes, C. A</creator><creator>Bonifazi, C</creator><creator>Borges, H. 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C ; Kemp, E ; Lessa, A ; Lichtenstein, G ; Machado, A. A ; Makler, M ; Marra, V ; Matheus, R. D ; Mercadante, P. G ; de Melo, T. B ; Nishi, C ; Nepomuceno, A ; Novaes, S. F ; Pimentel, V. L ; Pinheiro, P. R. D ; Pires, C. A ; Queiroz, A. R ; Queiroz, F. S ; ~Rangel, M. ~S ; Rodrigues, D. C ; Rodrigues, J. G ; de Souza, V ; da Silva, P. S. Rodrigues ; Siqueira, C ; Segreto, E ; Sanchez-Vega, B. L ; Rosenfeld, R ; Santos, J. R. L ; Santos, A. C. O ; Silva, R ; Sokolowska, D ; Teles, P. R ; Tomei, T. R. F. P ; Valdiviesso, G. 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A</creatorcontrib><creatorcontrib>Vasconcelos, P</creatorcontrib><creatorcontrib>Viana, A</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Abdalla, E</au><au>Albuquerque, I. F. M</au><au>Alves, A</au><au>Barosi, L</au><au>Bazetto, M. C. Q</au><au>Batista, R. C</au><au>Bernardes, C. A</au><au>Bonifazi, C</au><au>Borges, H. A</au><au>Brito, F. A</au><au>Caramês, T. R. P</au><au>Casarini, L</au><au>Cogollo, D</au><au>Dias, A. G</au><au>Esmaili, A</au><au>Ferreira, M. M</au><au>da Silveira, G. Gil</au><au>Guzzo, M. M</au><au>Hadjimichef, D</au><au>de Holanda, P. C</au><au>Kemp, E</au><au>Lessa, A</au><au>Lichtenstein, G</au><au>Machado, A. A</au><au>Makler, M</au><au>Marra, V</au><au>Matheus, R. D</au><au>Mercadante, P. G</au><au>de Melo, T. B</au><au>Nishi, C</au><au>Nepomuceno, A</au><au>Novaes, S. F</au><au>Pimentel, V. L</au><au>Pinheiro, P. R. D</au><au>Pires, C. A</au><au>Queiroz, A. R</au><au>Queiroz, F. S</au><au>~Rangel, M. ~S</au><au>Rodrigues, D. C</au><au>Rodrigues, J. G</au><au>de Souza, V</au><au>da Silva, P. S. Rodrigues</au><au>Siqueira, C</au><au>Segreto, E</au><au>Sanchez-Vega, B. L</au><au>Rosenfeld, R</au><au>Santos, J. R. L</au><au>Santos, A. C. O</au><au>Silva, R</au><au>Sokolowska, D</au><au>Teles, P. R</au><au>Tomei, T. R. F. P</au><au>Valdiviesso, G. A</au><au>Vasconcelos, P</au><au>Viana, A</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Brazilian Community Report on Dark Matter</atitle><date>2019-12-20</date><risdate>2019</risdate><abstract>This white paper summarizes the activities of the Brazilian community
concerning dark matter physics and highlights the importance of financial
support to Brazilian groups that are deeply involved in experimental
endeavours. The flagships of the Brazilian dark matter program are the
Cherenkov Telescope Array, DARKSIDE, SBN and LHC experiments, but we emphasize
that smaller experiments such as DAMIC and CONNIE constitute important probes
to dark sectors as well and should receive special attention. Small
experimental projects showing the potential to probe new regions of parameter
space of dark matter models are encouraged. On the theoretical and
phenomenological side, some groups are devoted to astrophysical aspects such as
the dark matter density profile while others explore the signature of dark
matter models at colliders, direct and indirect detection experiments. In
summary, the Brazilian dark matter community that was born not long ago has
grown tremendously in the past years and now plays an important role in the
hunt for a dark matter particle.</abstract><doi>10.48550/arxiv.1912.10076</doi><oa>free_for_read</oa></addata></record> |
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| identifier | DOI: 10.48550/arxiv.1912.10076 |
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| language | eng |
| recordid | cdi_arxiv_primary_1912_10076 |
| source | arXiv.org |
| subjects | Physics - Cosmology and Nongalactic Astrophysics Physics - High Energy Astrophysical Phenomena Physics - High Energy Physics - Phenomenology |
| title | Brazilian Community Report on Dark Matter |
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