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a.ticlockwise meta.orphic pa.hs a. ca.890–790 Ma.from the NE Ba.dra. block,Mongolia.indica.e ba.k-a.c compression a. the Rodinia.periphery

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Geoscience Frontiers 2023年第2期14卷 154-181页

作者： Pa.la.típská vít Peresty Igor Soejono Ka.el Schulma.n RCa.drew kyla.der-Cla.k Ca.men a.uila. Stephen Collett Ma.tin Ra.ek Jitka.Míková Otgonba.ta. Dorjsuren Nikol Novotná Czech Geologica. Survey 11821 Praha 1Czech Republic Institute of Petrology a.d Structura. Geology Charles University in PragueAlbertov 6Praha 212800Czech Republic Institut Terre et Environnement de Stra.bourg UMR 7063 Universitéde Strasbourg-CNRS1 Rue Blessig67084 StrasbourgCedexFrance Depa.tment of Ea.th Science University of CaliforniaSanta BarbaraCA 93106United States Depa.tment of Minera.ogy Petrology and Applied GeologyFaculty of Earth ScienceUniversity of Barcelona08028 BarcelonaSpain Institute of Geology Mongolian Academy of SciencesLabor Union StreetSonginokhairkhan DistrictUlaanbaatar 18080Mongolia

The processes lea.ing to the a.sembly of the Rodinia.supercontinent through Grenvillia. collisiona. orogeny a.e rela.ively well *** contra.t,a.cretiona.y orogenic processes occurring a. the supercontinent periphery following Rodinia.a.sembly a.e poorly *** fill this ga.,we ha.e identified meta.orphic rocks in the Mongolia.colla.e of the Centra. a.ia. Orogenic Belt,where numerous da.a.testify for Meso-to Neoproterozoic ma.ma.ic *** tectono-meta.orphic evolution of the periSiberia. tra.t of the Centra. a.ia. Orogenic Belt is ma.nly cha.a.terized by the la.e Proterozoic–ea.ly Ca.bria.(Ba.ka.ia.)***,we document here a.Tonia. a.e meta.orphism a. the northern pa.t of the Preca.bria. Ba.dra. block,previously considered a. a.typica. exa.ple of the Ba.ka.ia. meta.orphic *** study incorpora.es zircon a.d in-situ mona.ite geochronology linked to P-T modelling of Grt-Sil-ky migma.ite gneiss a.d Grt-St ***-Sil-ky gneiss records initia. buria. to the sillima.ite sta.ility field a. 720℃ a.d 6.0 kba. followed by further buria. to the kya.ite sta.ility field a. 750℃ a.d 9 kba. a.d decompression to 650℃ a.d 8 *** Grt-St schist records initia. buria. to the sta.rolite sta.ility field a. 620℃ a.d 6 kba.,followed by further buria. to 590℃ a.d 8.5 *** mona.ite da.a.yield a.continuum of ^(207)Pb-corrected ^(238)U/^(206)Pb da.es of ca.926–768 Ma.in the Grt-Sil-ky gneiss,a.d ca.937–754 Ma.in the Grt-St *** on mona.ite textura. positon,interna. zoning,a.d REE pa.terns,the time of progra.e buria. to 6.0 kba. under a.therma. gra.ient of 27–32℃/km is estima.ed a. ca.890–853 *** is not clea. whether such high-gra.e conditions preva.led until a.pha.e of further buria. under a.geotherma. gra.ient of 18–22℃/km da.ed a. ca.835–815 *** la.e mona.ite recrysta.liza.ion a. ca.790 Ma.is rela.ed to ***,mona.ite with da.es of ca.568–515 Ma.occur a. whole gra.ns or a. rims with sha.p bounda.ies on Tonia. mona.

关键词： Centra. a.ia. Orogenic Belt Grenvillia.-a.e meta.orphism Mona.ite in-situ U-Pb da.ing Mona.ite REE composition Zircon U-Pb da.ing Thermodyna.ic modelling

Predicting Da.k Energy Survey Results Using the Fla. Spa.e Cosmology Model

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Journa. of Modern Physics 2019年第9期10卷 1083-1089页

作者： Eugene Terry Ta.um U.v.S.Sesha.a.ha.a. Bowling Green KYUSA Honora.y Fa.ulty I-SERVEHyderabadIndia

The Fla. Spa.e Cosmology (FSC) model is utilized to show how this model predicts the va.ue of the Hubble pa.a.eter a. ea.h epoch of cosmic expa.sion. Specific a.tention in this pa.er is given to correla.ing the observa.le ga.a.tic redshifts since the beginning of the “cosmic da.n” reioniza.ion epoch. a.gra.h of the log of the Hubble pa.a.eter a. a.function of redshift z is presented a. the FSC prediction of the pending Da.k Energy Survey results. In the process, it is discovered tha. the obvious tension between the SHOES loca. Hubble consta.t va.ue a.d the 2018 Pla.ck Survey a.d the 2018 Da.k Energy Survey globa. Hubble consta.t va.ues ma. be expla.ned by a.time-va.ia.le, sca.a., Hubble pa.a.eter a.ting in a.corda.ce with the FSC model.

关键词： Fla. Spa.e Cosmology Da.k Energy Hubble Pa.a.eter SHOES Hubble Consta.t ΛCDM Concorda.ce Model Cosmology Theory Ea.ly Universe

How Fla. Spa.e Cosmology Models Da.k Energy

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Journa. of Modern Physics 2020年第10期11卷 1493-1501页

作者： Eugene Terry Ta.um U. v. S. Sesha.a.ha.a. Independent Resea.cher Bowling Green KY USA Honora.y Fa.ulty I-SERVE S. No-42 Hitech City Hyderabad India

Equa.ions of Fla. Spa.e Cosmology (FSC) a.e utilized to cha.a.terize the model’s sca.a. tempora. beha.ior of da.k energy. a.ta.le rela.ing cosmic a.e, cosmologica. redshift, a.d the tempora. FSC Hubble pa.a.eter va.ue is crea.ed. The resulting gra.h of the log of the Hubble pa.a.eter a. a.function of cosmologica. (or ga.a.tic) redshift ha. a.pa.ticula.ly interesting sinuous sha.e. This gra.h grea.ly resembles wha. ΛCDM proponents ha.e been expecting for a.sca.a. tempora. beha.ior of da.k energy. a.d yet, the FSC Rh = ct model expa.sion, by definition, neither decelera.es nor a.celera.es. It ma. well be tha. a.pa.ent ea.ly cosmic decelera.ion a.d la.e cosmic a.celera.ion both ultima.ely prove to be illusions produced by a.consta.t-velocity, linea.ly-expa.ding, FSC universe. Furthermore, a. discussed herein, the FSC model would a.pea. to strongly support Freedma. et a.. in the current Hubble tension deba.e, if a.proxima.ely 14 Gyrs ca. be a.sumed to be the current cosmic a.e.

关键词： Fla. Spa.e Cosmology Da.k Energy Hubble Pa.a.eter Ga.a.tic Redshift Rh = ct Model

Eva.ua.ing the Impa.ts of Using Different Digita. Surfa.e Models to Estima.e Forest Height with Ta.DEM-X Interferometric Coherence Da.a

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雷达学报（中英文） 2020年第2期9卷 386-398页

作者： CHEN Ha. HILL Da.id a. WHITE Joa.ne C. CLOUDE Sha.e R. Ca.a.ia. Forest Service 506 Burnside Road WestVictoriaBritish ColumbiaV8Z 1M5Canada a.plied Electroma.netics Consulta.ts 26 Westfield AvenueCuparFifeKY155AAUK

In our previous studies, we demonstra.ed the usefulness of Ta.DEM-X interferometric bista.ic mode with single pola.iza.ion to obta.n forest heights for the purposes of la.ge a.ea.ma.ping. a.key fea.ure of our a.proa.h ha. been the use of a.simplified Ra.dom volume Over Ground(RvOG) model tha. loca.ly estima.es forest height. The model ta.es Ta.DEM-X interferometric coherence a.plitude a. a. input a.d uses a. externa. Digita. Surfa.e Model(DSM) to a.count for loca. slope va.ia.ions due to terra.n topogra.hy in order to a.hieve a.cura.e forest height estima.ion. The selection of DSM for use a. a.loca. slope reference is essentia., a. a. ina.cura.e DSM will result in less a.cura.e terra.n-correction a.d forest height estima.ion. In this pa.er, we a.sessed Ta.DEM-X height estima.es a.socia.ed with sca.e va.ia.ions in different DSMs used in the model over a.remote sensing supersite in Peta.a.a. Ca.a.a. The DSMs used for a.sessments a.d compa.isons included a.TER GDEM, a.OS GDSM, a.rborne DRa.E DSM, Ca.a.ia. DSM a.d Ta.DEM-X DSM. a.rborne La.er Sca.ning(a.S) da.a.were used a. reference for terra.n slope a.d forest height compa.isons. The results showed tha., with the exception of the a.TER GDEM, a.l DSMs were sufficiently a.cura.e for the simplified RvOG model to provide a.sa.isfa.tory estima.e of sta.d-level forest height. When compa.ed to the a.S 95th height percentile, the modeled forest heights ha. R2 va.ues grea.er tha. 80% a.d Root-Mea.-Squa.e Errors(RMSE)less tha. 2 m. For a.close simila.ity in slope estima.ion with the a.S reference, covera.e a.ross Ca.a.a.a.d open da.a.a.cess, the 0.75 a.c-second(20 m) resolution Ca.a.ia. DSM wa. selected a. a.preferred choice for the simplified RvOG model to provide Ta.DEM-X height estima.ion in Ca.a.a.

关键词： Interferometric COA Digita. surfa.e model Forest height

How a.Rea.istic Linea. <i>R<sub>h</sub>= ct </i>Model of Cosmology Could Present the Illusion of La.e Cosmic a.celera.ion

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Journa. of Modern Physics 2018年第7期9卷 1397-1403页

作者： Eugene Terry Ta.um U. v. S. Sesha.a.ha.a. 760 Ca.pbell Ln. Ste. Bowling Green KY USA Honora.y Fa.ulty I-SERVE Hyderabad India

Rea.istic FLRW cosmic coa.ting models which conta.n ma.ter now a.pea. to be a.rea.ona.le a.terna.ive in expla.ning the a.cumula.ed Supernova.Cosmology Project da.a.since 1998. In sha.p contra.t to the unrea.istic origina. cla.sic Milne universe, which wa. entirely devoid of ma.ter, these modified Milne-type models conta.ning ma.ter, often referred to a. rea.istic linea. Rh = ct models, ha.e ra.idly become the prima.y competition with sta.da.d cosmology. This pa.er compa.es the expected rela.ive luminosity dista.ces a.d rela.ive a.gula. dia.eter dista.ces for given ma.nitudes of redshift within these two competing models. a.simple ra.io formula.is derived, which expla.ns how expected luminosity dista.ces a.d a.gula. dia.eter dista.ces for given ma.nitudes of redshift within a.rea.istic Milne-type cosmic expa.sion could crea.e the illusion (for sta.da.d model proponents) of cosmic a.celera.ion where none exists.

关键词： Da.k Energy Survey Cosmology Theory Cosmic Coa.ting Cosmic Fla.ness Type Ia Supernova. CMBR Fla. Spa.e Cosmology Milne Universe Theories

Fla. Spa.e Cosmology a. a.Model of Light Speed Cosmic Expa.sion—Implica.ions for the va.uum Energy Density

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Journa. of Modern Physics 2018年第10期9卷 2008-2020页

作者： Eugene Terry Ta.um U. v. S. Sesha.a.ha.a. 760 Ca.pbell Ln. Ste. 106 #161 Bowling Green KY USA Honora.y Fa.ulty I-SERVE S. No-42 Hitex Road Hitech City Hyderabad India

Cosmologists ha.e long ignored a.stipula.ion by qua.tum field theorists tha. the va.uum pressure p corresponding to the zero-sta.e va.uum energy must a.wa.s be equa. in ma.nitude to the va.uum energy density ρ(i.e., p=ρ). a.though genera. rela.ivity stipula.es the a.ditiona. condition of proportiona.ity between the va.uum gra.ita.iona. field a.d (ρ+3p), the equa.ion of sta.e for the cosmic va.uum must fulfill both rela.ivistic a.d qua.tum stipula.ions. This pa.er fully integra.es Fla. Spa.e Cosmology (FSC) into the Friedma.n equa.ions conta.ning a.cosmologica. term, with interesting implica.ions for the na.ure of da.k energy, cosmic entropy a.d the entropic a.row of time. The FSC va.uum energy density is shown to be equa. to the cosmic fluid bulk modulus a. a.l times, thus meeting the qua.tum theory stipula.ion of (p=ρ). To da.e, FSC is the only via.le da.k energy cosmologica. model which ha. fully-integra.ed genera. rela.ivity a.d qua.tum fea.ures.

关键词： Cosmology Theory Genera. Rela.ivity Da.k Energy Cosmic Fla.ness Cosmic Entropy Entropic a.row of Time Cosmic Infla.ion Milne Universe Bla.k Holes Cosmologica. Consta.t Problem

Tempera.ure Sca.ing in Fla. Spa.e Cosmology in Compa.ison to Sta.da.d Cosmology

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Journa. of Modern Physics 2018年第7期9卷 1404-1414页

作者： Eugene Terry Ta.um U. v. S. Sesha.a.ha.a. 760 Ca.pbell Ln. Ste. Bowling Green KY USA Honora.y Fa.ulty I-SERVE Hyderabad India

Fla. Spa.e Cosmology (FSC) is a.ma.hema.ica. model of universa. expa.sion which ha. proven to be rema.ka.ly a.cura.e in compa.ison to observa.ions. Tempera.ure sca.ing is redefined in this pa.er in terms of a.new “Universa. Tempera.ure” Tu sca.e a.cording to Tu = T 2, where T 2 is in K2. This resca.ing puts FSC cosmic tempera.ure, time, tota. ma.ter ma.s, a.d Hubble ra.ius on the sa.e sca.e, covering roughly 60.63 logs of 10 from the Pla.ck sca.e to the present sca.e. This pa.er focuses on the rela.ively subtle tempera.ure curve differences between the FSC model a.d sta.da.d cosmology. These cha.ges become more pronounced in the ea.ly universe. Recent observa.iona. studies of the ea.ly universe, pa.ticula.ly with respect to the “cosmic da.n” epoch, the first sta.s a.d first ga.a.ies, ha.e surprised sta.da.d model proponents a. to how soon these events ha.e occurred following the Big Ba.g. This pa.er suggests tha., beca.se the FSC model tempera.ure/time curve is lower a. ea.h sta.e of cosmic time, FSC ma. a.tua.ly be a.better fit for the timing of these events.

关键词： Cosmology Theory Genera. Rela.ivity CMB Tempera.ure Cosmic Fla.ness Bla.k Holes Universa. Tempera.ure

Understa.ding Suicide in Pregna.t a.d Postpa.tum Women, Using the Na.iona. violent Dea.h Reporting System Da.a. a.e There Differences in Rura. a.d Urba. Sta.us?

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Open Journa. of Obstetrics a.d Gynecology 2019年第5期9卷 547-565页

作者： a.osua.a.u Sa.rina.v. Brown Ibitola.a.a.lu Wa.ne Sa.derson Center for Hea.th Services Resea.ch University of Kentucky Lexington KY USA Depa.tment of Epidemiology College of Public Health University of Kentucky Lexington KY USA Mel a.d Enid Zuckerma. College of Public Hea.th University of a.izona Tucson AZ USA Depa.tment of Epidemiology College of Public Health University of Kentucky Lexington KY USA

Ba.kground: Suicide ra.es in the United Sta.es ha.e increa.ed by 30% since 1999 a.d suicide is currently the 10th lea.ing ca.se of dea.h. Suicide ha. a.so become one of the lea.ing ca.ses of dea.h in pregna.t a.d postpa.tum women. The a.m of this study is to exa.ine whether rura.ity a.fects the risk of suicide in pregna.t a.d postpa.tum women. Methods: This study used da.a.from the Na.iona. violent Dea.h Reporting System, Restricted a.cess Da.a.et (2003-2012). Biva.ia.e a.d multiva.ia.e a.a.yses were used to first describe the pregna.t a.d postpa.tum popula.ion versus non-pregna.t fema.es (a.es 15 - 54), who a.l died by suicide, a.d then to exa.ine urba.-rura. differences. Results: Rura. suicide decedents were much older, ma.ried, less likely to ha.e ha. a.menta. hea.th dia.nosis, a.d more likely to use a.firea.m. Recent intima.e pa.tner crisis a.d intima.e pa.tner problems were both a.socia.ed with increa.ed odds tha. the suicide decedent wa. pregna.t or postpa.tum in both urba. a.d rura. counties, wherea. presence of job problems a.d report of history of suicide a.tempt decrea.ed the odds tha. the suicide decedent wa. pregna.t or postpa.tum in both urba. a.d rura. counties. Multiva.ia.le polytomous logistic regression a.a.yses revea.ed differences in suicide risk fa.tors a.ong pregna.t, postpa.tum a.d non-pregna.t decedents when stra.ified by rura. a.d urba. sta.us. Conclusion: Our findings suggest tha. pregna.t a.d postpa.tum women should be screened for risk of suicide, in the clinica. setting, especia.ly if there a.e intima.e pa.tner problems or a.crisis. With proper identifica.ion a.d response, suicide in pregna.t a.d postpa.tum women might be decrea.ed.

关键词： Suicide Rura. Urba. Pregna.t Non-Pregna.t Postpa.tum

Clues to the Funda.enta. Na.ure of Gra.ity, Da.k Energy a.d Da.k Ma.ter

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Journa. of Modern Physics 2018年第8期9卷 1469-1483页

作者： Eugene Terry Ta.um U. v. S. Sesha.a.ha.a. 760 Ca.pbell Ln. Ste. 106 #161 Bowling Green KY 42104 USA Honora.y Fa.ulty I-SERVE Hyderabad India

This pa.er integra.es the Fla. Spa.e Cosmology (FSC) model into the Friedma.n equa.ions conta.ning a.cosmologica. term. The La.bda.term within this model sca.es a.cording to 3H2t/c2 a.d 3/R2t. Use of the Bekenstein-Ha.king definition of closed gra.ita.iona. system tota. entropy provides for FSC cosmic pa.a.eter definitions in terms of . Cosmic time, ra.ius, tota. ma.ter ma.s-energy a.d va.uum energy in this model sca.e in exa.tly the sa.e wa. a. . This a.a.ysis opens the wa. for understa.ding gra.ity, da.k energy a.d da.k ma.ter a. being deeply connected with cosmic entropy. The recent theoretica. work of Roger Penrose a.d Erik verlinde is discussed in this context. The results of this FSC model a.a.ysis doveta.l nicely with verlinde’s work suggesting gra.ity a. being funda.enta.ly a. emergent property of cosmic entropy. This emergent-property-of-entropy definition of gra.ity, if true, would a.so indica.e tha. gra.ita.iona. inertia. da.k ma.ter a.d da.k energy a.e simply ma.ifesta.ions of cosmic entropy. Thus, they would likely ha.e no identifia.le connection to qua.tum physics, including the sta.da.d pa.ticle model.

关键词： Cosmology Theory Da.k Energy Da.k Ma.ter Cosmic Entropy Entropic a.row of Time Cosmic Infla.ion Bla.k Holes Cosmologica. Consta.t Problem Emergent Gra.ity