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<?xml version="1.0" encoding="UTF-8"?> <articles> <article xmlns:xlink="http://www.w3.org/1999/xlink/"> <front> <journal-meta> <journal-title>Phys. Rev. Accel. Beams</journal-title> <abbrev-journal-title>Phys. Rev. Accel. Beams</abbrev-journal-title> <issn/> </journal-meta> <article-meta> <title-group> <article-title>Energy deposition studies for the Upgrade II of LHCb at the CERN Large Hadron Collider</article-title> </title-group> <contrib-group> <contrib contrib-type="author"> <name> <surname>Ciccotelli</surname> <given-names>Alessia</given-names> </name> <aff> <institution>CERN</institution> </aff> <aff> <institution>U. Manchester (main)</institution> </aff> <aff> <institution>Cockcroft Inst. Accel. Sci. Tech.</institution> </aff> </contrib> <contrib contrib-type="author"> <name> <surname>Appleby</surname> <given-names>Robert B.</given-names> </name> <aff> <institution>U. Manchester (main)</institution> </aff> <aff> <institution>Cockcroft Inst. Accel. Sci. Tech.</institution> </aff> </contrib> <contrib contrib-type="author"> <name> <surname>Cerutti</surname> <given-names>Francesco</given-names> </name> <aff> <institution>CERN</institution> </aff> </contrib> <contrib contrib-type="author"> <name> <surname>Buffet</surname> <given-names>Kevin</given-names> </name> <aff> <institution>CERN</institution> </aff> </contrib> <contrib contrib-type="author"> <name> <surname>Butin</surname> <given-names>Francois</given-names> </name> <aff> <institution>CERN</institution> </aff> </contrib> <contrib contrib-type="author"> <name> <surname>Corti</surname> <given-names>Gloria</given-names> </name> <aff> <institution>CERN</institution> </aff> </contrib> <contrib contrib-type="author"> <name> <surname>Esposito</surname> <given-names>Luigi Salvatore</given-names> </name> <aff> <institution>CERN</institution> </aff> </contrib> <contrib contrib-type="author"> <name> <surname>Garcia Alia</surname> <given-names>Ruben</given-names> </name> <aff> <institution>CERN</institution> </aff> </contrib> <contrib contrib-type="author"> <name> <surname>Karacson</surname> <given-names>Matthias</given-names> </name> <aff> <institution>CERN</institution> </aff> </contrib> <contrib contrib-type="author"> <name> <surname>Lerner</surname> <given-names>Giuseppe</given-names> </name> <aff> <institution>CERN</institution> </aff> </contrib> <contrib contrib-type="author"> <name> <surname>Wehrle</surname> <given-names>Maud</given-names> </name> <aff> <institution>CERN</institution> </aff> </contrib> <contrib contrib-type="author"> <name> <surname>Prelipcean</surname> <given-names>Daniel</given-names> </name> <aff> <institution>CERN</institution> </aff> <aff> <institution>Munich, Tech. U.</institution> </aff> </contrib> </contrib-group> <pub-date pub-type="pub"> <year>2024</year> </pub-date> <volume>27</volume> <fpage/> <lpage/> <self-uri xlink:href="http://cds.cern.ch/record/2875966"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/D2_360_rev1.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/HEH_UL84.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/MBXWS_1R8.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/Detector_UpgradeII.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/2310.08281.pdf"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/DS_dose.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/Dose_triplet_D1_rev1.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/MBXWH_1L8_360.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/scale.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/R_factor.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/TAS.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/D2_IPface_down.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/TI8_IR8_lhcb_wall_4.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/TAS_Q1.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/DS_dose360.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/Dose_at_max_D2_combined.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/LHCb-to-2037.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/MBXWS_1R8_360.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/plot_2023_right_01_log.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/MBXWS_shielding_range.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/effect.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/MBXWS_1L8_360.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/D2_IPface_up.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/Lumi_UpgradeII_my.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/TAS1.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/D1_4R8_shielding_2023.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/plot_2023_right_02_log.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/Power_LHCb_ATLAS.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/PeakPower_right_triplet_D1.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/MBXWS_shielding_range_real.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/SHIELD_D1.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/Pea_power_D2.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/TI8_IR8_lhcb_3D_prompt_run3_wall3.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/Lumi_UpgradeII_TDR.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/Dose_right_triplet_D101.png"/> <self-uri xlink:href="http://cds.cern.ch/record/2875966/files/Publication.pdf"/> </article-meta> <abstract>The Upgrade II of the Large Hadron Collider beauty (LHCb) experiment is proposed to be installed during the CERN Long Shutdown 4, aiming to operate LHCb at <math display="inline"><mrow><mn>1.5</mn><mo>×</mo><msup><mrow><mn>10</mn></mrow><mrow><mn>34</mn></mrow></msup><mtext> </mtext><mtext> </mtext><msup><mrow><mi>cm</mi></mrow><mrow><mo>−</mo><mn>2</mn></mrow></msup><mtext> </mtext><msup><mrow><mi mathvariant="normal">s</mi></mrow><mrow><mo>−</mo><mn>1</mn></mrow></msup></mrow></math> that is 75 times its design luminosity [1] and reaching an integrated luminosity of about <math display="inline"><mrow><mn>400</mn><mtext> </mtext><mtext> </mtext><msup><mi>fb</mi><mrow><mo>−</mo><mn>1</mn></mrow></msup></mrow></math> by the end of the High Luminosity LHC era. This increase of the data sample at LHCb is an unprecedented opportunity for heavy flavor physics measurements. A first upgrade of LHCb (Upgrade I), completed in 2022, has already implemented important changes of the LHCb detector and, for the Upgrade II, further detector improvements of the tracking system, the particle identification system and the online and trigger infrastructure are being considered. Such a luminosity increase will have an impact not only on the LHCb detector but also on the LHC magnets, cryogenics, and electronic equipment placed in the insertion region 8. In fact, the LHCb experiment was conceived to work at a much lower luminosity than ATLAS and CMS, implying minor requirements for protection of the LHC elements from the collision debris, and therefore, a different layout around the interaction point. The Upgrade I has already implied the installation of an absorber for the neutral particle debris (TANB). However, the luminosity target proposed for this second upgrade requires to review the layout of the entire insertion region in order to ensure safe operation of the LHC magnets and to mitigate the risk of failure of the electronic devices. The objective of this paper is to provide an overview of the implications of the Upgrade II of LHCb in the experimental cavern and in the tunnel with a focus on the LHCb detector, electronic devices, and accelerator magnets. This proves that the Upgrade II luminosity goal can be sustained with the implementation of protection systems for magnets and electronics. The electronics placed in the experimental areas and in the cavern needs to be protected to mitigate a single event effect risk, which may imply recurring downtime of the LHC. On the other hand, protection for the first quadrupole of the final focus triplet and for the separation dipole are needed to prevent their quench and to reach the desired lifetime. Moreover, the normal-conducting compensators require the installation of shielding to limit their head coil degradation.</abstract> </front> <article-type>research-article</article-type> <ref/> </article> </articles>