Exact time-localized solutions in Vacuum String Field Theory
Nucl.Phys. B715 (2005) 413-439 We address the problem of finding star algebra projectors that exhibit localized time profiles. We use the double Wick rotation method, starting from an Euclidean (unconventional) lump solution, which is characterized by the Neumann matrix being the conventional one fo...
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| creator | Bonora, L Maccaferri, C Santos, R. J. Scherer Tolla, D. D |
| description | Nucl.Phys. B715 (2005) 413-439 We address the problem of finding star algebra projectors that exhibit
localized time profiles. We use the double Wick rotation method, starting from
an Euclidean (unconventional) lump solution, which is characterized by the
Neumann matrix being the conventional one for the continuous spectrum, while
the inverse of the conventional one for the discrete spectrum. This is still a
solution of the projector equation and we show that, after inverse
Wick-rotation, its time profile has the desired localized time dependence. We
study it in detail in the low energy regime (field theory limit) and in the
extreme high energy regime (tensionless limit) and show its similarities with
the rolling tachyon solution. |
| doi_str_mv | 10.48550/arxiv.hep-th/0409063 |
| format | Article |
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localized time profiles. We use the double Wick rotation method, starting from
an Euclidean (unconventional) lump solution, which is characterized by the
Neumann matrix being the conventional one for the continuous spectrum, while
the inverse of the conventional one for the discrete spectrum. This is still a
solution of the projector equation and we show that, after inverse
Wick-rotation, its time profile has the desired localized time dependence. We
study it in detail in the low energy regime (field theory limit) and in the
extreme high energy regime (tensionless limit) and show its similarities with
the rolling tachyon solution.</description><identifier>DOI: 10.48550/arxiv.hep-th/0409063</identifier><language>eng</language><subject>Physics - High Energy Physics - Theory</subject><creationdate>2004-09</creationdate><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,778,883</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/hep-th/0409063$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.hep-th/0409063$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1016/j.nuclphysb.2005.02.040$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Bonora, L</creatorcontrib><creatorcontrib>Maccaferri, C</creatorcontrib><creatorcontrib>Santos, R. J. Scherer</creatorcontrib><creatorcontrib>Tolla, D. D</creatorcontrib><title>Exact time-localized solutions in Vacuum String Field Theory</title><description>Nucl.Phys. B715 (2005) 413-439 We address the problem of finding star algebra projectors that exhibit
localized time profiles. We use the double Wick rotation method, starting from
an Euclidean (unconventional) lump solution, which is characterized by the
Neumann matrix being the conventional one for the continuous spectrum, while
the inverse of the conventional one for the discrete spectrum. This is still a
solution of the projector equation and we show that, after inverse
Wick-rotation, its time profile has the desired localized time dependence. We
study it in detail in the low energy regime (field theory limit) and in the
extreme high energy regime (tensionless limit) and show its similarities with
the rolling tachyon solution.</description><subject>Physics - High Energy Physics - Theory</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2004</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNpjYJA1NNAzsTA1NdBPLKrILNPLSC3QLcnQNzAxsDQwM-ZksHGtSEwuUSjJzE3VzclPTszJrEpNUSjOzyktyczPK1bIzFMIS0wuLc1VCC4pysxLV3DLTM1JUQjJSM0vquRhYE1LzClO5YXS3AzKbq4hzh66YLviC4oycxOLKuOBdsaXZMRD7TQmThUASgs7Sw</recordid><startdate>20040906</startdate><enddate>20040906</enddate><creator>Bonora, L</creator><creator>Maccaferri, C</creator><creator>Santos, R. J. Scherer</creator><creator>Tolla, D. D</creator><scope>GOX</scope></search><sort><creationdate>20040906</creationdate><title>Exact time-localized solutions in Vacuum String Field Theory</title><author>Bonora, L ; Maccaferri, C ; Santos, R. J. Scherer ; Tolla, D. D</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-arxiv_primary_hep_th_04090633</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2004</creationdate><topic>Physics - High Energy Physics - Theory</topic><toplevel>online_resources</toplevel><creatorcontrib>Bonora, L</creatorcontrib><creatorcontrib>Maccaferri, C</creatorcontrib><creatorcontrib>Santos, R. J. Scherer</creatorcontrib><creatorcontrib>Tolla, D. D</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Bonora, L</au><au>Maccaferri, C</au><au>Santos, R. J. Scherer</au><au>Tolla, D. D</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Exact time-localized solutions in Vacuum String Field Theory</atitle><date>2004-09-06</date><risdate>2004</risdate><abstract>Nucl.Phys. B715 (2005) 413-439 We address the problem of finding star algebra projectors that exhibit
localized time profiles. We use the double Wick rotation method, starting from
an Euclidean (unconventional) lump solution, which is characterized by the
Neumann matrix being the conventional one for the continuous spectrum, while
the inverse of the conventional one for the discrete spectrum. This is still a
solution of the projector equation and we show that, after inverse
Wick-rotation, its time profile has the desired localized time dependence. We
study it in detail in the low energy regime (field theory limit) and in the
extreme high energy regime (tensionless limit) and show its similarities with
the rolling tachyon solution.</abstract><doi>10.48550/arxiv.hep-th/0409063</doi><oa>free_for_read</oa></addata></record> |
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| title | Exact time-localized solutions in Vacuum String Field Theory |
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