TeV scale implications of non commutative space time in laboratory frame with polarized beams
We analyze e + e − → γγ , e − γ → e − γ and γγ → e + e − processes within the Seiberg-Witten expanded noncommutative scenario using polarized beams. With unpolarized beams the leading order effects of non commutativity starts from second order in non commutative (NC) parameter i.e. O (Θ 2 ), w...
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| Veröffentlicht in: | The journal of high energy physics 2011-07, Vol.2011 (7), Article 24 |
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| container_title | The journal of high energy physics |
| container_volume | 2011 |
| creator | Garg, Sumit K. Shreecharan, T. Das, P. K. Deshpande, N. G. Rajasekaran, G. |
| description | We analyze
e
+
e
−
→
γγ
,
e
−
γ
→
e
−
γ
and
γγ
→
e
+
e
−
processes within the Seiberg-Witten expanded noncommutative scenario using polarized beams. With unpolarized beams the leading order effects of non commutativity starts from second order in non commutative (NC) parameter i.e.
O
(Θ
2
), while with polarized beams these corrections appear at first order (
O
(Θ)) in cross section. The corrections in Compton case can probe the magnetic component
while in Pair production and Pair annihilation probe the electric component
of NC parameter. We include the effects of earth rotation in our analysis. This study is done by investigating the effects of non commutativity on different time averaged cross section observables. The results which also depends on the position of the collider, can provide clear and distinct signatures of the model testable at the International Linear Collider (ILC). |
| doi_str_mv | 10.1007/JHEP07(2011)024 |
| format | Article |
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e
+
e
−
→
γγ
,
e
−
γ
→
e
−
γ
and
γγ
→
e
+
e
−
processes within the Seiberg-Witten expanded noncommutative scenario using polarized beams. With unpolarized beams the leading order effects of non commutativity starts from second order in non commutative (NC) parameter i.e.
O
(Θ
2
), while with polarized beams these corrections appear at first order (
O
(Θ)) in cross section. The corrections in Compton case can probe the magnetic component
while in Pair production and Pair annihilation probe the electric component
of NC parameter. We include the effects of earth rotation in our analysis. This study is done by investigating the effects of non commutativity on different time averaged cross section observables. The results which also depends on the position of the collider, can provide clear and distinct signatures of the model testable at the International Linear Collider (ILC).</description><identifier>ISSN: 1029-8479</identifier><identifier>EISSN: 1029-8479</identifier><identifier>DOI: 10.1007/JHEP07(2011)024</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer-Verlag</publisher><subject>Beams (radiation) ; Classical and Quantum Gravitation ; Commutativity ; Cross-sections ; Earth rotation ; Electric components ; Elementary Particles ; High energy physics ; Model testing ; Pair production ; Parameters ; Physics ; Physics and Astronomy ; Quantum Field Theories ; Quantum Field Theory ; Quantum Physics ; Relativity Theory ; String Theory ; Superconducting supercolliders</subject><ispartof>The journal of high energy physics, 2011-07, Vol.2011 (7), Article 24</ispartof><rights>SISSA, Trieste, Italy 2011</rights><rights>SISSA, Trieste, Italy 2011.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c310t-5f35229f6cb0c9bc1629e158811bfc94bd7862d042ca975fff7f959c30ca36973</citedby><cites>FETCH-LOGICAL-c310t-5f35229f6cb0c9bc1629e158811bfc94bd7862d042ca975fff7f959c30ca36973</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/JHEP07(2011)024$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://doi.org/10.1007/JHEP07(2011)024$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,776,780,27903,27904,41099,41467,42168,42536,51297,51554</link.rule.ids><linktorsrc>$$Uhttps://doi.org/10.1007/JHEP07(2011)024$$EView_record_in_Springer_Nature$$FView_record_in_$$GSpringer_Nature</linktorsrc></links><search><creatorcontrib>Garg, Sumit K.</creatorcontrib><creatorcontrib>Shreecharan, T.</creatorcontrib><creatorcontrib>Das, P. K.</creatorcontrib><creatorcontrib>Deshpande, N. G.</creatorcontrib><creatorcontrib>Rajasekaran, G.</creatorcontrib><title>TeV scale implications of non commutative space time in laboratory frame with polarized beams</title><title>The journal of high energy physics</title><addtitle>J. High Energ. Phys</addtitle><description>We analyze
e
+
e
−
→
γγ
,
e
−
γ
→
e
−
γ
and
γγ
→
e
+
e
−
processes within the Seiberg-Witten expanded noncommutative scenario using polarized beams. With unpolarized beams the leading order effects of non commutativity starts from second order in non commutative (NC) parameter i.e.
O
(Θ
2
), while with polarized beams these corrections appear at first order (
O
(Θ)) in cross section. The corrections in Compton case can probe the magnetic component
while in Pair production and Pair annihilation probe the electric component
of NC parameter. We include the effects of earth rotation in our analysis. This study is done by investigating the effects of non commutativity on different time averaged cross section observables. The results which also depends on the position of the collider, can provide clear and distinct signatures of the model testable at the International Linear Collider (ILC).</description><subject>Beams (radiation)</subject><subject>Classical and Quantum Gravitation</subject><subject>Commutativity</subject><subject>Cross-sections</subject><subject>Earth rotation</subject><subject>Electric components</subject><subject>Elementary Particles</subject><subject>High energy physics</subject><subject>Model testing</subject><subject>Pair production</subject><subject>Parameters</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum Field Theories</subject><subject>Quantum Field Theory</subject><subject>Quantum Physics</subject><subject>Relativity Theory</subject><subject>String Theory</subject><subject>Superconducting supercolliders</subject><issn>1029-8479</issn><issn>1029-8479</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2011</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNp1kE1LAzEQhoMoWKtnrwEvelg7yX5kc5TSWqWgh-pNQjZNdMvuZk1Spf56U1bQi6cZhud9Bx6EzglcEwA2uV_MHoFdUiDkCmh2gEYEKE_KjPHDP_sxOvF-A0BywmGEXlb6GXslG43rtm9qJUNtO4-twZ3tsLJtuw3x9qGx76XSONRtRDvcyMo6GazbYeNkvH3W4Q33tpGu_tJrXGnZ-lN0ZGTj9dnPHKOn-Ww1XSTLh9u76c0yUSmBkOQmzSnlplAVKF4pUlCuSV6WhFRG8axas7Kga8iokpzlxhhmeM5VCkqmBWfpGF0Mvb2z71vtg9jYreviS0FTXtKUQrGnJgOlnPXeaSN6V7fS7QQBsXcoBodi71BEhzEBQ8JHsnvV7rf3v8g3n7Rz5A</recordid><startdate>20110701</startdate><enddate>20110701</enddate><creator>Garg, Sumit K.</creator><creator>Shreecharan, T.</creator><creator>Das, P. 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G. ; Rajasekaran, G.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c310t-5f35229f6cb0c9bc1629e158811bfc94bd7862d042ca975fff7f959c30ca36973</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2011</creationdate><topic>Beams (radiation)</topic><topic>Classical and Quantum Gravitation</topic><topic>Commutativity</topic><topic>Cross-sections</topic><topic>Earth rotation</topic><topic>Electric components</topic><topic>Elementary Particles</topic><topic>High energy physics</topic><topic>Model testing</topic><topic>Pair production</topic><topic>Parameters</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quantum Field Theories</topic><topic>Quantum Field Theory</topic><topic>Quantum Physics</topic><topic>Relativity Theory</topic><topic>String Theory</topic><topic>Superconducting supercolliders</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Garg, Sumit K.</creatorcontrib><creatorcontrib>Shreecharan, T.</creatorcontrib><creatorcontrib>Das, P. K.</creatorcontrib><creatorcontrib>Deshpande, N. G.</creatorcontrib><creatorcontrib>Rajasekaran, G.</creatorcontrib><collection>CrossRef</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><jtitle>The journal of high energy physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Garg, Sumit K.</au><au>Shreecharan, T.</au><au>Das, P. K.</au><au>Deshpande, N. G.</au><au>Rajasekaran, G.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>TeV scale implications of non commutative space time in laboratory frame with polarized beams</atitle><jtitle>The journal of high energy physics</jtitle><stitle>J. High Energ. Phys</stitle><date>2011-07-01</date><risdate>2011</risdate><volume>2011</volume><issue>7</issue><artnum>24</artnum><issn>1029-8479</issn><eissn>1029-8479</eissn><abstract>We analyze
e
+
e
−
→
γγ
,
e
−
γ
→
e
−
γ
and
γγ
→
e
+
e
−
processes within the Seiberg-Witten expanded noncommutative scenario using polarized beams. With unpolarized beams the leading order effects of non commutativity starts from second order in non commutative (NC) parameter i.e.
O
(Θ
2
), while with polarized beams these corrections appear at first order (
O
(Θ)) in cross section. The corrections in Compton case can probe the magnetic component
while in Pair production and Pair annihilation probe the electric component
of NC parameter. We include the effects of earth rotation in our analysis. This study is done by investigating the effects of non commutativity on different time averaged cross section observables. The results which also depends on the position of the collider, can provide clear and distinct signatures of the model testable at the International Linear Collider (ILC).</abstract><cop>Berlin/Heidelberg</cop><pub>Springer-Verlag</pub><doi>10.1007/JHEP07(2011)024</doi><oa>free_for_read</oa></addata></record> |
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| identifier | ISSN: 1029-8479 |
| ispartof | The journal of high energy physics, 2011-07, Vol.2011 (7), Article 24 |
| issn | 1029-8479 1029-8479 |
| language | eng |
| recordid | cdi_proquest_journals_2398232067 |
| source | Springer Nature OA Free Journals |
| subjects | Beams (radiation) Classical and Quantum Gravitation Commutativity Cross-sections Earth rotation Electric components Elementary Particles High energy physics Model testing Pair production Parameters Physics Physics and Astronomy Quantum Field Theories Quantum Field Theory Quantum Physics Relativity Theory String Theory Superconducting supercolliders |
| title | TeV scale implications of non commutative space time in laboratory frame with polarized beams |
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