Towards the light front variables for high energy production processes

Abstract. Scale invariant presentation of inclusive spectra in terms of light front variables is proposed. The variables introduced go over to the well-known scaling variables $x_F = 2 p_z /\sqrt s$ and $x_T =2 p_T / \sqrt s$ in the high $p_z$ and high $P_T$ limits respectively. Some surface is foun...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Amaglobeli, N.S. [verfasserIn] Esakia, S.M. Garsevanishvilil, V.R. Kuratashvili, G.O. Kutsidi, N.K. Kvatadze, R.A. Tevzadze, Yu V. Topuria, T.P.

Format:	Artikel
Sprache:	Englisch

Erschienen:	1999

Schlagwörter:	Statistical Model Phase Space Production Process Energy Production High Limit

Anmerkung:	© Springer-Verlag Berlin Heidelberg 1999

Übergeordnetes Werk:	Enthalten in: The European physical journal / C - Springer-Verlag, 1998, 8(1999), 4 vom: Mai, Seite 603-607
Übergeordnetes Werk:	volume:8 ; year:1999 ; number:4 ; month:05 ; pages:603-607

Links:	Volltext

DOI / URN:	10.1007/s100529901056

Katalog-ID:	OLC2069062023

Internformat


LEADER	01000caa a22002652 4500
001	OLC2069062023
003	DE-627
005	20230502163603.0
007	tu
008	200819s1999 xx \|\|\|\|\| 00\| \|\|eng c
024	7		\|a 10.1007/s100529901056 \|2 doi
035			\|a (DE-627)OLC2069062023
035			\|a (DE-He213)s100529901056-p
040			\|a DE-627 \|b ger \|c DE-627 \|e rakwb
041			\|a eng
082	0	4	\|a 530 \|q VZ
082	0	4	\|a 530 \|q VZ
100	1		\|a Amaglobeli, N.S. \|e verfasserin \|4 aut
245	1	0	\|a Towards the light front variables for high energy production processes
264		1	\|c 1999
336			\|a Text \|b txt \|2 rdacontent
337			\|a ohne Hilfsmittel zu benutzen \|b n \|2 rdamedia
338			\|a Band \|b nc \|2 rdacarrier
500			\|a © Springer-Verlag Berlin Heidelberg 1999
520			\|a Abstract. Scale invariant presentation of inclusive spectra in terms of light front variables is proposed. The variables introduced go over to the well-known scaling variables $x_F = 2 p_z /\sqrt s$ and $x_T =2 p_T / \sqrt s$ in the high $p_z$ and high $P_T$ limits respectively. Some surface is found in the phase space of produced $\pi^\pm$-mesons in the inclusive reaction $\bar pp \to \pi^\pm X$ at 22.4 GeV/c, which separates two groups of particles with significantly different characteristics. In one of these regions a naive statistical model seems to be in a good agreement with data, whereas it fails in the second region.
650		4	\|a Statistical Model
650		4	\|a Phase Space
650		4	\|a Production Process
650		4	\|a Energy Production
650		4	\|a High Limit
700	1		\|a Esakia, S.M. \|4 aut
700	1		\|a Garsevanishvilil, V.R. \|4 aut
700	1		\|a Kuratashvili, G.O. \|4 aut
700	1		\|a Kutsidi, N.K. \|4 aut
700	1		\|a Kvatadze, R.A. \|4 aut
700	1		\|a Tevzadze, Yu V. \|4 aut
700	1		\|a Topuria, T.P. \|4 aut
773	0	8	\|i Enthalten in \|t The European physical journal / C \|d Springer-Verlag, 1998 \|g 8(1999), 4 vom: Mai, Seite 603-607 \|w (DE-627)235469777 \|w (DE-600)1397769-6 \|w (DE-576)061879150 \|x 1434-6044 \|7 nnns
773	1	8	\|g volume:8 \|g year:1999 \|g number:4 \|g month:05 \|g pages:603-607
856	4	1	\|u https://doi.org/10.1007/s100529901056 \|z lizenzpflichtig \|3 Volltext
912			\|a GBV_USEFLAG_A
912			\|a SYSFLAG_A
912			\|a GBV_OLC
912			\|a SSG-OLC-PHY
912			\|a GBV_ILN_11
912			\|a GBV_ILN_20
912			\|a GBV_ILN_21
912			\|a GBV_ILN_22
912			\|a GBV_ILN_30
912			\|a GBV_ILN_32
912			\|a GBV_ILN_40
912			\|a GBV_ILN_62
912			\|a GBV_ILN_70
912			\|a GBV_ILN_130
912			\|a GBV_ILN_267
912			\|a GBV_ILN_2006
912			\|a GBV_ILN_2018
912			\|a GBV_ILN_2409
912			\|a GBV_ILN_4029
912			\|a GBV_ILN_4082
912			\|a GBV_ILN_4126
912			\|a GBV_ILN_4277
912			\|a GBV_ILN_4306
912			\|a GBV_ILN_4310
912			\|a GBV_ILN_4319
951			\|a AR
952			\|d 8 \|j 1999 \|e 4 \|c 05 \|h 603-607

Indexfelder

author_variant	n a na s e se v g vg g k gk n k nk r k rk y v t yv yvt t t tt
matchkey_str	article:14346044:1999----::oadteihfotaibefrihnryr
hierarchy_sort_str	1999
publishDate	1999
allfields	10.1007/s100529901056 doi (DE-627)OLC2069062023 (DE-He213)s100529901056-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Amaglobeli, N.S. verfasserin aut Towards the light front variables for high energy production processes 1999 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag Berlin Heidelberg 1999 Abstract. Scale invariant presentation of inclusive spectra in terms of light front variables is proposed. The variables introduced go over to the well-known scaling variables $x_F = 2 p_z /\sqrt s$ and $x_T =2 p_T / \sqrt s$ in the high $p_z$ and high $P_T$ limits respectively. Some surface is found in the phase space of produced $\pi^\pm$-mesons in the inclusive reaction $\bar pp \to \pi^\pm X$ at 22.4 GeV/c, which separates two groups of particles with significantly different characteristics. In one of these regions a naive statistical model seems to be in a good agreement with data, whereas it fails in the second region. Statistical Model Phase Space Production Process Energy Production High Limit Esakia, S.M. aut Garsevanishvilil, V.R. aut Kuratashvili, G.O. aut Kutsidi, N.K. aut Kvatadze, R.A. aut Tevzadze, Yu V. aut Topuria, T.P. aut Enthalten in The European physical journal / C Springer-Verlag, 1998 8(1999), 4 vom: Mai, Seite 603-607 (DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150 1434-6044 nnns volume:8 year:1999 number:4 month:05 pages:603-607 https://doi.org/10.1007/s100529901056 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_30 GBV_ILN_32 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_2409 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4126 GBV_ILN_4277 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4319 AR 8 1999 4 05 603-607
spelling	10.1007/s100529901056 doi (DE-627)OLC2069062023 (DE-He213)s100529901056-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Amaglobeli, N.S. verfasserin aut Towards the light front variables for high energy production processes 1999 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag Berlin Heidelberg 1999 Abstract. Scale invariant presentation of inclusive spectra in terms of light front variables is proposed. The variables introduced go over to the well-known scaling variables $x_F = 2 p_z /\sqrt s$ and $x_T =2 p_T / \sqrt s$ in the high $p_z$ and high $P_T$ limits respectively. Some surface is found in the phase space of produced $\pi^\pm$-mesons in the inclusive reaction $\bar pp \to \pi^\pm X$ at 22.4 GeV/c, which separates two groups of particles with significantly different characteristics. In one of these regions a naive statistical model seems to be in a good agreement with data, whereas it fails in the second region. Statistical Model Phase Space Production Process Energy Production High Limit Esakia, S.M. aut Garsevanishvilil, V.R. aut Kuratashvili, G.O. aut Kutsidi, N.K. aut Kvatadze, R.A. aut Tevzadze, Yu V. aut Topuria, T.P. aut Enthalten in The European physical journal / C Springer-Verlag, 1998 8(1999), 4 vom: Mai, Seite 603-607 (DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150 1434-6044 nnns volume:8 year:1999 number:4 month:05 pages:603-607 https://doi.org/10.1007/s100529901056 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_30 GBV_ILN_32 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_2409 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4126 GBV_ILN_4277 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4319 AR 8 1999 4 05 603-607
allfields_unstemmed	10.1007/s100529901056 doi (DE-627)OLC2069062023 (DE-He213)s100529901056-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Amaglobeli, N.S. verfasserin aut Towards the light front variables for high energy production processes 1999 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag Berlin Heidelberg 1999 Abstract. Scale invariant presentation of inclusive spectra in terms of light front variables is proposed. The variables introduced go over to the well-known scaling variables $x_F = 2 p_z /\sqrt s$ and $x_T =2 p_T / \sqrt s$ in the high $p_z$ and high $P_T$ limits respectively. Some surface is found in the phase space of produced $\pi^\pm$-mesons in the inclusive reaction $\bar pp \to \pi^\pm X$ at 22.4 GeV/c, which separates two groups of particles with significantly different characteristics. In one of these regions a naive statistical model seems to be in a good agreement with data, whereas it fails in the second region. Statistical Model Phase Space Production Process Energy Production High Limit Esakia, S.M. aut Garsevanishvilil, V.R. aut Kuratashvili, G.O. aut Kutsidi, N.K. aut Kvatadze, R.A. aut Tevzadze, Yu V. aut Topuria, T.P. aut Enthalten in The European physical journal / C Springer-Verlag, 1998 8(1999), 4 vom: Mai, Seite 603-607 (DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150 1434-6044 nnns volume:8 year:1999 number:4 month:05 pages:603-607 https://doi.org/10.1007/s100529901056 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_30 GBV_ILN_32 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_2409 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4126 GBV_ILN_4277 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4319 AR 8 1999 4 05 603-607
allfieldsGer	10.1007/s100529901056 doi (DE-627)OLC2069062023 (DE-He213)s100529901056-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Amaglobeli, N.S. verfasserin aut Towards the light front variables for high energy production processes 1999 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag Berlin Heidelberg 1999 Abstract. Scale invariant presentation of inclusive spectra in terms of light front variables is proposed. The variables introduced go over to the well-known scaling variables $x_F = 2 p_z /\sqrt s$ and $x_T =2 p_T / \sqrt s$ in the high $p_z$ and high $P_T$ limits respectively. Some surface is found in the phase space of produced $\pi^\pm$-mesons in the inclusive reaction $\bar pp \to \pi^\pm X$ at 22.4 GeV/c, which separates two groups of particles with significantly different characteristics. In one of these regions a naive statistical model seems to be in a good agreement with data, whereas it fails in the second region. Statistical Model Phase Space Production Process Energy Production High Limit Esakia, S.M. aut Garsevanishvilil, V.R. aut Kuratashvili, G.O. aut Kutsidi, N.K. aut Kvatadze, R.A. aut Tevzadze, Yu V. aut Topuria, T.P. aut Enthalten in The European physical journal / C Springer-Verlag, 1998 8(1999), 4 vom: Mai, Seite 603-607 (DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150 1434-6044 nnns volume:8 year:1999 number:4 month:05 pages:603-607 https://doi.org/10.1007/s100529901056 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_30 GBV_ILN_32 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_2409 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4126 GBV_ILN_4277 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4319 AR 8 1999 4 05 603-607
allfieldsSound	10.1007/s100529901056 doi (DE-627)OLC2069062023 (DE-He213)s100529901056-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Amaglobeli, N.S. verfasserin aut Towards the light front variables for high energy production processes 1999 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag Berlin Heidelberg 1999 Abstract. Scale invariant presentation of inclusive spectra in terms of light front variables is proposed. The variables introduced go over to the well-known scaling variables $x_F = 2 p_z /\sqrt s$ and $x_T =2 p_T / \sqrt s$ in the high $p_z$ and high $P_T$ limits respectively. Some surface is found in the phase space of produced $\pi^\pm$-mesons in the inclusive reaction $\bar pp \to \pi^\pm X$ at 22.4 GeV/c, which separates two groups of particles with significantly different characteristics. In one of these regions a naive statistical model seems to be in a good agreement with data, whereas it fails in the second region. Statistical Model Phase Space Production Process Energy Production High Limit Esakia, S.M. aut Garsevanishvilil, V.R. aut Kuratashvili, G.O. aut Kutsidi, N.K. aut Kvatadze, R.A. aut Tevzadze, Yu V. aut Topuria, T.P. aut Enthalten in The European physical journal / C Springer-Verlag, 1998 8(1999), 4 vom: Mai, Seite 603-607 (DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150 1434-6044 nnns volume:8 year:1999 number:4 month:05 pages:603-607 https://doi.org/10.1007/s100529901056 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_30 GBV_ILN_32 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_2409 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4126 GBV_ILN_4277 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4319 AR 8 1999 4 05 603-607
language	English
source	Enthalten in The European physical journal / C 8(1999), 4 vom: Mai, Seite 603-607 volume:8 year:1999 number:4 month:05 pages:603-607
sourceStr	Enthalten in The European physical journal / C 8(1999), 4 vom: Mai, Seite 603-607 volume:8 year:1999 number:4 month:05 pages:603-607
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Statistical Model Phase Space Production Process Energy Production High Limit
dewey-raw	530
isfreeaccess_bool	false
container_title	The European physical journal / C
authorswithroles_txt_mv	Amaglobeli, N.S. @@aut@@ Esakia, S.M. @@aut@@ Garsevanishvilil, V.R. @@aut@@ Kuratashvili, G.O. @@aut@@ Kutsidi, N.K. @@aut@@ Kvatadze, R.A. @@aut@@ Tevzadze, Yu V. @@aut@@ Topuria, T.P. @@aut@@
publishDateDaySort_date	1999-05-01T00:00:00Z
hierarchy_top_id	235469777
dewey-sort	3530
id	OLC2069062023
language_de	englisch
fullrecord	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2069062023</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502163603.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s1999 xx \|\|\|\|\| 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s100529901056</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2069062023</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s100529901056-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Amaglobeli, N.S.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Towards the light front variables for high energy production processes</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1999</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Springer-Verlag Berlin Heidelberg 1999</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract. Scale invariant presentation of inclusive spectra in terms of light front variables is proposed. The variables introduced go over to the well-known scaling variables $x_F = 2 p_z /\sqrt s$ and $x_T =2 p_T / \sqrt s$ in the high $p_z$ and high $P_T$ limits respectively. Some surface is found in the phase space of produced $\pi^\pm$-mesons in the inclusive reaction $\bar pp \to \pi^\pm X$ at 22.4 GeV/c, which separates two groups of particles with significantly different characteristics. In one of these regions a naive statistical model seems to be in a good agreement with data, whereas it fails in the second region.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Statistical Model</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Phase Space</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Production Process</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Energy Production</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">High Limit</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Esakia, S.M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Garsevanishvilil, V.R.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kuratashvili, G.O.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kutsidi, N.K.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kvatadze, R.A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tevzadze, Yu V.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Topuria, T.P.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">The European physical journal / C</subfield><subfield code="d">Springer-Verlag, 1998</subfield><subfield code="g">8(1999), 4 vom: Mai, Seite 603-607</subfield><subfield code="w">(DE-627)235469777</subfield><subfield code="w">(DE-600)1397769-6</subfield><subfield code="w">(DE-576)061879150</subfield><subfield code="x">1434-6044</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:8</subfield><subfield code="g">year:1999</subfield><subfield code="g">number:4</subfield><subfield code="g">month:05</subfield><subfield code="g">pages:603-607</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/s100529901056</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_20</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_21</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_30</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_32</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_62</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_130</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_267</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2006</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2018</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2409</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4029</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4082</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4126</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4277</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4306</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4310</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4319</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">8</subfield><subfield code="j">1999</subfield><subfield code="e">4</subfield><subfield code="c">05</subfield><subfield code="h">603-607</subfield></datafield></record></collection>
author	Amaglobeli, N.S.
spellingShingle	Amaglobeli, N.S. ddc 530 misc Statistical Model misc Phase Space misc Production Process misc Energy Production misc High Limit Towards the light front variables for high energy production processes
authorStr	Amaglobeli, N.S.
ppnlink_with_tag_str_mv	@@773@@(DE-627)235469777
format	Article
dewey-ones	530 - Physics
delete_txt_mv	keep
author_role	aut aut aut aut aut aut aut aut
collection	OLC
remote_str	false
illustrated	Not Illustrated
issn	1434-6044
topic_title	530 VZ Towards the light front variables for high energy production processes Statistical Model Phase Space Production Process Energy Production High Limit
topic	ddc 530 misc Statistical Model misc Phase Space misc Production Process misc Energy Production misc High Limit
topic_unstemmed	ddc 530 misc Statistical Model misc Phase Space misc Production Process misc Energy Production misc High Limit
topic_browse	ddc 530 misc Statistical Model misc Phase Space misc Production Process misc Energy Production misc High Limit
format_facet	Aufsätze Gedruckte Aufsätze
format_main_str_mv	Text Zeitschrift/Artikel
carriertype_str_mv	nc
hierarchy_parent_title	The European physical journal / C
hierarchy_parent_id	235469777
dewey-tens	530 - Physics
hierarchy_top_title	The European physical journal / C
isfreeaccess_txt	false
familylinks_str_mv	(DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150
title	Towards the light front variables for high energy production processes
ctrlnum	(DE-627)OLC2069062023 (DE-He213)s100529901056-p
title_full	Towards the light front variables for high energy production processes
author_sort	Amaglobeli, N.S.
journal	The European physical journal / C
journalStr	The European physical journal / C
lang_code	eng
isOA_bool	false
dewey-hundreds	500 - Science
recordtype	marc
publishDateSort	1999
contenttype_str_mv	txt
container_start_page	603
author_browse	Amaglobeli, N.S. Esakia, S.M. Garsevanishvilil, V.R. Kuratashvili, G.O. Kutsidi, N.K. Kvatadze, R.A. Tevzadze, Yu V. Topuria, T.P.
container_volume	8
class	530 VZ
format_se	Aufsätze
author-letter	Amaglobeli, N.S.
doi_str_mv	10.1007/s100529901056
dewey-full	530
title_sort	towards the light front variables for high energy production processes
title_auth	Towards the light front variables for high energy production processes
abstract	Abstract. Scale invariant presentation of inclusive spectra in terms of light front variables is proposed. The variables introduced go over to the well-known scaling variables $x_F = 2 p_z /\sqrt s$ and $x_T =2 p_T / \sqrt s$ in the high $p_z$ and high $P_T$ limits respectively. Some surface is found in the phase space of produced $\pi^\pm$-mesons in the inclusive reaction $\bar pp \to \pi^\pm X$ at 22.4 GeV/c, which separates two groups of particles with significantly different characteristics. In one of these regions a naive statistical model seems to be in a good agreement with data, whereas it fails in the second region. © Springer-Verlag Berlin Heidelberg 1999
abstractGer	Abstract. Scale invariant presentation of inclusive spectra in terms of light front variables is proposed. The variables introduced go over to the well-known scaling variables $x_F = 2 p_z /\sqrt s$ and $x_T =2 p_T / \sqrt s$ in the high $p_z$ and high $P_T$ limits respectively. Some surface is found in the phase space of produced $\pi^\pm$-mesons in the inclusive reaction $\bar pp \to \pi^\pm X$ at 22.4 GeV/c, which separates two groups of particles with significantly different characteristics. In one of these regions a naive statistical model seems to be in a good agreement with data, whereas it fails in the second region. © Springer-Verlag Berlin Heidelberg 1999
abstract_unstemmed	Abstract. Scale invariant presentation of inclusive spectra in terms of light front variables is proposed. The variables introduced go over to the well-known scaling variables $x_F = 2 p_z /\sqrt s$ and $x_T =2 p_T / \sqrt s$ in the high $p_z$ and high $P_T$ limits respectively. Some surface is found in the phase space of produced $\pi^\pm$-mesons in the inclusive reaction $\bar pp \to \pi^\pm X$ at 22.4 GeV/c, which separates two groups of particles with significantly different characteristics. In one of these regions a naive statistical model seems to be in a good agreement with data, whereas it fails in the second region. © Springer-Verlag Berlin Heidelberg 1999
collection_details	GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_30 GBV_ILN_32 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_2409 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4126 GBV_ILN_4277 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4319
container_issue	4
title_short	Towards the light front variables for high energy production processes
url	https://doi.org/10.1007/s100529901056
remote_bool	false
author2	Esakia, S.M. Garsevanishvilil, V.R. Kuratashvili, G.O. Kutsidi, N.K. Kvatadze, R.A. Tevzadze, Yu V. Topuria, T.P.
author2Str	Esakia, S.M. Garsevanishvilil, V.R. Kuratashvili, G.O. Kutsidi, N.K. Kvatadze, R.A. Tevzadze, Yu V. Topuria, T.P.
ppnlink	235469777
mediatype_str_mv	n
isOA_txt	false
hochschulschrift_bool	false
doi_str	10.1007/s100529901056
up_date	2024-07-03T20:46:46.869Z
_version_	1803592250812268544
fullrecord_marcxml	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2069062023</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502163603.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s1999 xx \|\|\|\|\| 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s100529901056</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2069062023</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s100529901056-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Amaglobeli, N.S.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Towards the light front variables for high energy production processes</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1999</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Springer-Verlag Berlin Heidelberg 1999</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract. Scale invariant presentation of inclusive spectra in terms of light front variables is proposed. The variables introduced go over to the well-known scaling variables $x_F = 2 p_z /\sqrt s$ and $x_T =2 p_T / \sqrt s$ in the high $p_z$ and high $P_T$ limits respectively. Some surface is found in the phase space of produced $\pi^\pm$-mesons in the inclusive reaction $\bar pp \to \pi^\pm X$ at 22.4 GeV/c, which separates two groups of particles with significantly different characteristics. In one of these regions a naive statistical model seems to be in a good agreement with data, whereas it fails in the second region.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Statistical Model</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Phase Space</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Production Process</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Energy Production</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">High Limit</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Esakia, S.M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Garsevanishvilil, V.R.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kuratashvili, G.O.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kutsidi, N.K.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kvatadze, R.A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tevzadze, Yu V.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Topuria, T.P.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">The European physical journal / C</subfield><subfield code="d">Springer-Verlag, 1998</subfield><subfield code="g">8(1999), 4 vom: Mai, Seite 603-607</subfield><subfield code="w">(DE-627)235469777</subfield><subfield code="w">(DE-600)1397769-6</subfield><subfield code="w">(DE-576)061879150</subfield><subfield code="x">1434-6044</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:8</subfield><subfield code="g">year:1999</subfield><subfield code="g">number:4</subfield><subfield code="g">month:05</subfield><subfield code="g">pages:603-607</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/s100529901056</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_20</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_21</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_30</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_32</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_62</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_130</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_267</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2006</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2018</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2409</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4029</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4082</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4126</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4277</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4306</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4310</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4319</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">8</subfield><subfield code="j">1999</subfield><subfield code="e">4</subfield><subfield code="c">05</subfield><subfield code="h">603-607</subfield></datafield></record></collection>
score	7.4017944

Nicht das Richtige dabei?

Schreiben Sie uns!

Towards the light front variables for high energy production processes

Nicht das Richtige dabei?

Zugang & Verfügbarkeit

Vorhandene Bände

Nicht das Richtige dabei?