Revision 8

05 Jun 2011 - Main.VincenzoVagnoni

Line: 1 to 1

History of $\sin 2\beta$ predictions

Changed:

<
<

>
>

EPS - PDF - PNG - JPG - GIF

Changed:

<
<

From left to right, they correspond to the following papers:

dRLMPPPPS90 (de Rujula, Lusignoli, Masetti, Pich, Petrarca, Prades, Pugliese, Steger), LHC Workshop Proc., Vol. II, CERN 90-10, ECFA 90-133, DEC. 1990.
DDGN90 (Dib, Dunietz, Gilman, Nir), Phys. Rev. D41 (1990) 1522.
LMMR92 (Lusignoli, Martinelli, Maiani, Reina), Nucl. Phys. B369 (1992) 139.
AL94 (Ali, London), hep-ph/9405283.
CFMRS95 (Ciuchini, Franco, Martinelli, Reina, Silvestrini), Z. Phys C68 (1995) 239.
BBL96 (Buchalla, Buras, Lautenbacher), Rev. Mod. Phys. 68(1996), 1125.
AL96 (Ali, London), Nuovo Cimento 109A (1996) 957.
PPRS97 (Paganini, Parodi, Roudeau, Stocchi), Physica Scripta Vol. 58 (1998) 556-559.
BF97 (Buras, Fleischer), Adv. Ser. Direct. HEP 15 (1998) 65.
BPS98 (Parodi, Roudeau, Stocchi), Il Nuovo Cimento 112A (1999) 883.
PS98 (Schune, Plaszczynski), hep-ph/9911280.
AL99 (Ali, London) Eur. Phys. J. C9 (1999) 687.
CFGLM99 (Ciuchini, Franco, Giusti, Lubicz, Martinelli), Nucl.Phys. B573 (2000) 201.
CPRS99 (Caravaglios, Parodi, Roudeau, Stocchi), hep-ph/0002171.
M99 (Mele), Phys. Rev. D59 (1999) 113011.
CDFLMPRS00 (Ciuchini, D'Agostini, Franco, Lubicz, Martinelli, Parodi, Roudeau, Stocchi), JHEP 0107 (2001) 013.
B.et.al.00 (Bargiotti et al.), La Riv. del Nuovo Cimento Vol. 23 N3 (2000) 1.
HLLL00 (Hoecker, Laplace, Lacker, LeDiberder), Eur. Phys. J C21 (2001) 225.
and the value from this UTfit paper.

The dotted lines correspond to the 95% C.L. regions (the only information given in those papers). The larger bands (from year '99) correspond to values of $\sin 2\beta$ from direct measurements.

>
>

From left to right, they correspond to the following papers:

dRLMPPPPS90 (de Rujula, Lusignoli, Masetti, Pich, Petrarca, Prades, Pugliese, Steger), LHC Workshop Proc., Vol. II, CERN 90-10, ECFA 90-133, DEC. 1990.
DDGN90 (Dib, Dunietz, Gilman, Nir), Phys. Rev. D41 (1990) 1522.
LMMR92 (Lusignoli, Martinelli, Maiani, Reina), Nucl. Phys. B369 (1992) 139.
AL94 (Ali, London), hep-ph/9405283.
CFMRS95 (Ciuchini, Franco, Martinelli, Reina, Silvestrini), Z. Phys C68 (1995) 239.
BBL96 (Buchalla, Buras, Lautenbacher), Rev. Mod. Phys. 68(1996), 1125.
AL96 (Ali, London), Nuovo Cimento 109A (1996) 957.
PPRS97 (Paganini, Parodi, Roudeau, Stocchi), Physica Scripta Vol. 58 (1998) 556-559.
BF97 (Buras, Fleischer), Adv. Ser. Direct. HEP 15 (1998) 65.
BPS98 (Parodi, Roudeau, Stocchi), Il Nuovo Cimento 112A (1999) 883.
PS98 (Schune, Plaszczynski), hep-ph/9911280.
AL99 (Ali, London) Eur. Phys. J. C9 (1999) 687.
CFGLM99 (Ciuchini, Franco, Giusti, Lubicz, Martinelli), Nucl.Phys. B573 (2000) 201.
CPRS99 (Caravaglios, Parodi, Roudeau, Stocchi), hep-ph/0002171.
M99 (Mele), Phys. Rev. D59 (1999) 113011.
CDFLMPRS00 (Ciuchini, D'Agostini, Franco, Lubicz, Martinelli, Parodi, Roudeau, Stocchi), JHEP 0107 (2001) 013.
B.et.al.00 (Bargiotti et al.), La Riv. del Nuovo Cimento Vol. 23 N3 (2000) 1.
HLLL00 (Hoecker, Laplace, Lacker, LeDiberder), Eur. Phys. J C21 (2001) 225.
and the value from this UTfit paper.

The dotted lines correspond to the 95% C.L. regions (the only information given in those papers). The larger bands (from year '99) correspond to values of $\sin 2\beta$ from direct measurements.

Added:

>
>

History of $\Delta m_s$ predictions

Changed:

<
<

>
>

EPS - PDF - PNG - JPG - GIF

Changed:

<
<

From left to right, they correspond to the following papers:

AL94 (Ali, London), hep-ph/9405283.
BBL95 (Buchalla, Buras, Lautenbacher), Rev. Mod. Phys. 68(1996), 1125.
AL96 (Ali, London), Nuovo Cimento 109A (1996) 957.
PPRS97 (Paganini, Parodi, Roudeau, Stocchi), Physica Scripta Vol. 58 (1998) 556-559.
BF97 (Buras, Fleischer), Adv. Ser. Direct. HEP 15 (1998) 65.
BPS98 (Parodi, Roudeau, Stocchi), Il Nuovo Cimento 112A (1999) 883.
AL00 (Ali, London) Eur. Phys. J. C9 (1999) 687.
CDFLMPRS00 (Ciuchini, D'Agostini, Franco, Lubicz, Martinelli, Parodi, Roudeau, Stocchi), JHEP 0107 (2001) 013.
B.et.al.00 (Bargiotti et al.), La Riv. del Nuovo Cimento Vol. 23 N3 (2000) 1.
HLLL00 (Hoecker, Laplace, Lacker, LeDiberder?), Eur. Phys. J C21 (2001) 225.
M01 (Mele), hep-ph/0103040.
UTfit Collaboration.
CKMfitter Group.
UTfit Collaboration.

>
>

From left to right, they correspond to the following papers:

AL94 (Ali, London), hep-ph/9405283.
BBL95 (Buchalla, Buras, Lautenbacher), Rev. Mod. Phys. 68(1996), 1125.
AL96 (Ali, London), Nuovo Cimento 109A (1996) 957.
PPRS97 (Paganini, Parodi, Roudeau, Stocchi), Physica Scripta Vol. 58 (1998) 556-559.
BF97 (Buras, Fleischer), Adv. Ser. Direct. HEP 15 (1998) 65.
BPS98 (Parodi, Roudeau, Stocchi), Il Nuovo Cimento 112A (1999) 883.
AL00 (Ali, London) Eur. Phys. J. C9 (1999) 687.
CDFLMPRS00 (Ciuchini, D'Agostini, Franco, Lubicz, Martinelli, Parodi, Roudeau, Stocchi), JHEP 0107 (2001) 013.
B.et.al.00 (Bargiotti et al.), La Riv. del Nuovo Cimento Vol. 23 N3 (2000) 1.
HLLL00 (Hoecker, Laplace, Lacker, LeDiberder?), Eur. Phys. J C21 (2001) 225.
M01 (Mele), hep-ph/0103040.
UTfit Collaboration.
CKMfitter Group.
UTfit Collaboration.

The full (dotted) lines correspond to the 68% (95%) C.L. regions. The star indicates the present world average.

Changed:

<
<

>
>

Added:

>
>

15 years of $( \bar{\rho},~\bar{\eta} )$ predictions

Added:

>
>

Evolution from 1988 to 2003 of the allowed region in the $(\bar{\rho},~\bar{\eta} )$ plane (contours at 68% and 95% probability are indicated by continuous black curves).

Changed:

<
<

>
>

%ADDTOHEAD{"WebHome" text="

>
>

#marqueecontainer{ position: relative; width: 450px; height: 420px; background-color: %F4F5F6; overflow: hidden; border: 3px solid #F4F5F6; padding: 2px; padding-left: 4px;

"

>
>

#marqueecontainer2{ position: relative; width: 450px; height: 420px; background-color: %F4F5F6; overflow: hidden; border: 3px solid #F4F5F6; padding: 2px; padding-left: 4px; "

}%

Revision 7

15 May 2010 - Main.VincenzoVagnoni

Line: 1 to 1

History of $\sin 2\beta$ predictions

Changed:

<
<

[EPS format] [JPG format]

From left to right, they correspond to the following papers:

dRLMPPPPS90 (de Rujula, Lusignoli, Masetti, Pich, Petrarca, Prades, Pugliese, Steger), LHC Workshop Proc., Vol. II, CERN 90-10, ECFA 90-133, DEC. 1990.
DDGN90 (Dib, Dunietz, Gilman, Nir), Phys. Rev. D41 (1990) 1522.
LMMR92 (Lusignoli, Martinelli, Maiani, Reina), Nucl. Phys. B369 (1992) 139.
AL94 (Ali, London), hep-ph/9405283.
CFMRS95 (Ciuchini, Franco, Martinelli, Reina, Silvestrini), Z. Phys C68 (1995) 239.
BBL96 (Buchalla, Buras, Lautenbacher), Rev. Mod. Phys. 68(1996), 1125.
AL96 (Ali, London), Nuovo Cimento 109A (1996) 957.
PPRS97 (Paganini, Parodi, Roudeau, Stocchi), Physica Scripta Vol. 58 (1998) 556-559.
BF97 (Buras, Fleischer), Adv. Ser. Direct. HEP 15 (1998) 65.
BPS98 (Parodi, Roudeau, Stocchi), Il Nuovo Cimento 112A (1999) 883.
PS98 (Schune, Plaszczynski), hep-ph/9911280.
AL99 (Ali, London) Eur. Phys. J. C9 (1999) 687.
CFGLM99 (Ciuchini, Franco, Giusti, Lubicz, Martinelli), Nucl.Phys. B573 (2000) 201.
CPRS99 (Caravaglios, Parodi, Roudeau, Stocchi), hep-ph/0002171.
M99 (Mele), Phys. Rev. D59 (1999) 113011.
CDFLMPRS00 (Ciuchini, D'Agostini, Franco, Lubicz, Martinelli, Parodi, Roudeau, Stocchi), JHEP 0107 (2001) 013.
B.et.al.00 (Bargiotti et al.), La Riv. del Nuovo Cimento Vol. 23 N3 (2000) 1.
HLLL00 (Hoecker, Laplace, Lacker, LeDiberder), Eur. Phys. J C21 (2001) 225.
and the value from this UTfit paper.

The dotted lines correspond to the 95% C.L. regions (the only information given in those papers). The larger bands (from year '99) correspond to values of $\sin 2\beta$ from direct measurements.

>
>

Changed:

<
<

>
>

EPS - PDF - PNG - JPG - GIF

From left to right, they correspond to the following papers:

dRLMPPPPS90 (de Rujula, Lusignoli, Masetti, Pich, Petrarca, Prades, Pugliese, Steger), LHC Workshop Proc., Vol. II, CERN 90-10, ECFA 90-133, DEC. 1990.
DDGN90 (Dib, Dunietz, Gilman, Nir), Phys. Rev. D41 (1990) 1522.
LMMR92 (Lusignoli, Martinelli, Maiani, Reina), Nucl. Phys. B369 (1992) 139.
AL94 (Ali, London), hep-ph/9405283.
CFMRS95 (Ciuchini, Franco, Martinelli, Reina, Silvestrini), Z. Phys C68 (1995) 239.
BBL96 (Buchalla, Buras, Lautenbacher), Rev. Mod. Phys. 68(1996), 1125.
AL96 (Ali, London), Nuovo Cimento 109A (1996) 957.
PPRS97 (Paganini, Parodi, Roudeau, Stocchi), Physica Scripta Vol. 58 (1998) 556-559.
BF97 (Buras, Fleischer), Adv. Ser. Direct. HEP 15 (1998) 65.
BPS98 (Parodi, Roudeau, Stocchi), Il Nuovo Cimento 112A (1999) 883.
PS98 (Schune, Plaszczynski), hep-ph/9911280.
AL99 (Ali, London) Eur. Phys. J. C9 (1999) 687.
CFGLM99 (Ciuchini, Franco, Giusti, Lubicz, Martinelli), Nucl.Phys. B573 (2000) 201.
CPRS99 (Caravaglios, Parodi, Roudeau, Stocchi), hep-ph/0002171.
M99 (Mele), Phys. Rev. D59 (1999) 113011.
CDFLMPRS00 (Ciuchini, D'Agostini, Franco, Lubicz, Martinelli, Parodi, Roudeau, Stocchi), JHEP 0107 (2001) 013.
B.et.al.00 (Bargiotti et al.), La Riv. del Nuovo Cimento Vol. 23 N3 (2000) 1.
HLLL00 (Hoecker, Laplace, Lacker, LeDiberder), Eur. Phys. J C21 (2001) 225.
and the value from this UTfit paper.

The dotted lines correspond to the 95% C.L. regions (the only information given in those papers). The larger bands (from year '99) correspond to values of $\sin 2\beta$ from direct measurements.

History of $\Delta m_s$ predictions

Changed:

<
<

[EPS format] [JPG format]

>
>

EPS - PDF - PNG - JPG - GIF

From left to right, they correspond to the following papers:

AL94 (Ali, London), hep-ph/9405283.
BBL95 (Buchalla, Buras, Lautenbacher), Rev. Mod. Phys. 68(1996), 1125.
AL96 (Ali, London), Nuovo Cimento 109A (1996) 957.
PPRS97 (Paganini, Parodi, Roudeau, Stocchi), Physica Scripta Vol. 58 (1998) 556-559.
BF97 (Buras, Fleischer), Adv. Ser. Direct. HEP 15 (1998) 65.
BPS98 (Parodi, Roudeau, Stocchi), Il Nuovo Cimento 112A (1999) 883.
AL00 (Ali, London) Eur. Phys. J. C9 (1999) 687.
CDFLMPRS00 (Ciuchini, D'Agostini, Franco, Lubicz, Martinelli, Parodi, Roudeau, Stocchi), JHEP 0107 (2001) 013.
B.et.al.00 (Bargiotti et al.), La Riv. del Nuovo Cimento Vol. 23 N3 (2000) 1.
HLLL00 (Hoecker, Laplace, Lacker, LeDiberder?), Eur. Phys. J C21 (2001) 225.
M01 (Mele), hep-ph/0103040.
UTfit Collaboration.
CKMfitter Group.
UTfit Collaboration.

The full (dotted) lines correspond to the 68% (95%) C.L. regions. The star indicates the present world average.

Changed:

<
<

>
>

15 years of $( \bar{\rho},~\bar{\eta} )$ predictions

Evolution from 1988 to 2003 of the allowed region in the $(\bar{\rho},~\bar{\eta} )$ plane (contours at 68% and 95% probability are indicated by continuous black curves).

Changed:

<
<

>
>

Revision 6

06 Apr 2010 - Main.MarcoCiuchini

Line: 1 to 1

Changed:

<
<

>
>

Deleted:

<
<

History of $\sin 2\beta$ predictions

Changed:

<
<

[EPS format] [JPG format]

From left to right, they correspond to the following papers:

dRLMPPPPS90 (de Rujula, Lusignoli, Masetti, Pich, Petrarca, Prades, Pugliese, Steger), LHC Workshop Proc., Vol. II, CERN 90-10, ECFA 90-133, DEC. 1990.
DDGN90 (Dib, Dunietz, Gilman, Nir), Phys. Rev. D41 (1990) 1522.
LMMR92 (Lusignoli, Martinelli, Maiani, Reina), Nucl. Phys. B369 (1992) 139.
AL94 (Ali, London), hep-ph/9405283.
CFMRS95 (Ciuchini, Franco, Martinelli, Reina, Silvestrini), Z. Phys C68 (1995) 239.
BBL96 (Buchalla, Buras, Lautenbacher), Rev. Mod. Phys. 68(1996), 1125.
AL96 (Ali, London), Nuovo Cimento 109A (1996) 957.
PPRS97 (Paganini, Parodi, Roudeau, Stocchi), Physica Scripta Vol. 58 (1998) 556-559.
BF97 (Buras, Fleischer), Adv. Ser. Direct. HEP 15 (1998) 65.
BPS98 (Parodi, Roudeau, Stocchi), Il Nuovo Cimento 112A (1999) 883.
PS98 (Schune, Plaszczynski), hep-ph/9911280.
AL99 (Ali, London) Eur. Phys. J. C9 (1999) 687.
CFGLM99 (Ciuchini, Franco, Giusti, Lubicz, Martinelli), Nucl.Phys. B573 (2000) 201.
CPRS99 (Caravaglios, Parodi, Roudeau, Stocchi), hep-ph/0002171.
M99 (Mele), Phys. Rev. D59 (1999) 113011.
CDFLMPRS00 (Ciuchini, D'Agostini, Franco, Lubicz, Martinelli, Parodi, Roudeau, Stocchi), JHEP 0107 (2001) 013.
B.et.al.00 (Bargiotti et al.), La Riv. del Nuovo Cimento Vol. 23 N3 (2000) 1.
HLLL00 (Hoecker, Laplace, Lacker, LeDiberder), Eur. Phys. J C21 (2001) 225.
and the latest value from this UTfit paper.

The dotted lines correspond to the 95% C.L. regions (the only information given in those papers). The larger bands (from year '99) correspond to values of $\sin 2\beta$ from direct measurements.

>
>

History of $\sin 2\beta$ predictions

[EPS format] [JPG format]

From left to right, they correspond to the following papers:

dRLMPPPPS90 (de Rujula, Lusignoli, Masetti, Pich, Petrarca, Prades, Pugliese, Steger), LHC Workshop Proc., Vol. II, CERN 90-10, ECFA 90-133, DEC. 1990.
DDGN90 (Dib, Dunietz, Gilman, Nir), Phys. Rev. D41 (1990) 1522.
LMMR92 (Lusignoli, Martinelli, Maiani, Reina), Nucl. Phys. B369 (1992) 139.
AL94 (Ali, London), hep-ph/9405283.
CFMRS95 (Ciuchini, Franco, Martinelli, Reina, Silvestrini), Z. Phys C68 (1995) 239.
BBL96 (Buchalla, Buras, Lautenbacher), Rev. Mod. Phys. 68(1996), 1125.
AL96 (Ali, London), Nuovo Cimento 109A (1996) 957.
PPRS97 (Paganini, Parodi, Roudeau, Stocchi), Physica Scripta Vol. 58 (1998) 556-559.
BF97 (Buras, Fleischer), Adv. Ser. Direct. HEP 15 (1998) 65.
BPS98 (Parodi, Roudeau, Stocchi), Il Nuovo Cimento 112A (1999) 883.
PS98 (Schune, Plaszczynski), hep-ph/9911280.
AL99 (Ali, London) Eur. Phys. J. C9 (1999) 687.
CFGLM99 (Ciuchini, Franco, Giusti, Lubicz, Martinelli), Nucl.Phys. B573 (2000) 201.
CPRS99 (Caravaglios, Parodi, Roudeau, Stocchi), hep-ph/0002171.
M99 (Mele), Phys. Rev. D59 (1999) 113011.
CDFLMPRS00 (Ciuchini, D'Agostini, Franco, Lubicz, Martinelli, Parodi, Roudeau, Stocchi), JHEP 0107 (2001) 013.
B.et.al.00 (Bargiotti et al.), La Riv. del Nuovo Cimento Vol. 23 N3 (2000) 1.
HLLL00 (Hoecker, Laplace, Lacker, LeDiberder), Eur. Phys. J C21 (2001) 225.
and the value from this UTfit paper.

The dotted lines correspond to the 95% C.L. regions (the only information given in those papers). The larger bands (from year '99) correspond to values of $\sin 2\beta$ from direct measurements.

History of $\Delta m_s$ predictions

Added:

>
>

[EPS format] [JPG format]

From left to right, they correspond to the following papers:

AL94 (Ali, London), hep-ph/9405283.
BBL95 (Buchalla, Buras, Lautenbacher), Rev. Mod. Phys. 68(1996), 1125.
AL96 (Ali, London), Nuovo Cimento 109A (1996) 957.
PPRS97 (Paganini, Parodi, Roudeau, Stocchi), Physica Scripta Vol. 58 (1998) 556-559.
BF97 (Buras, Fleischer), Adv. Ser. Direct. HEP 15 (1998) 65.
BPS98 (Parodi, Roudeau, Stocchi), Il Nuovo Cimento 112A (1999) 883.
AL00 (Ali, London) Eur. Phys. J. C9 (1999) 687.
CDFLMPRS00 (Ciuchini, D'Agostini, Franco, Lubicz, Martinelli, Parodi, Roudeau, Stocchi), JHEP 0107 (2001) 013.
B.et.al.00 (Bargiotti et al.), La Riv. del Nuovo Cimento Vol. 23 N3 (2000) 1.
HLLL00 (Hoecker, Laplace, Lacker, LeDiberder?), Eur. Phys. J C21 (2001) 225.
M01 (Mele), hep-ph/0103040.
UTfit Collaboration.
CKMfitter Group.
UTfit Collaboration.

The full (dotted) lines correspond to the 68% (95%) C.L. regions. The star indicates the present world average.

Changed:

<
<

[EPS format] [JPG format]

From left to right, they correspond to the following papers:

AL94 (Ali, London), hep-ph/9405283.
BBL95 (Buchalla, Buras, Lautenbacher), Rev. Mod. Phys. 68(1996), 1125.
AL96 (Ali, London), Nuovo Cimento 109A (1996) 957.
PPRS97 (Paganini, Parodi, Roudeau, Stocchi), Physica Scripta Vol. 58 (1998) 556-559.
BF97 (Buras, Fleischer), Adv. Ser. Direct. HEP 15 (1998) 65.
BPS98 (Parodi, Roudeau, Stocchi), Il Nuovo Cimento 112A (1999) 883.
AL00 (Ali, London) Eur. Phys. J. C9 (1999) 687.
CDFLMPRS00 (Ciuchini, D'Agostini, Franco, Lubicz, Martinelli, Parodi, Roudeau, Stocchi), JHEP 0107 (2001) 013.
B.et.al.00 (Bargiotti et al.), La Riv. del Nuovo Cimento Vol. 23 N3 (2000) 1.
HLLL00 (Hoecker, Laplace, Lacker, LeDiberder?), Eur. Phys. J C21 (2001) 225.
M01 (Mele), hep-ph/0103040.
UTfit Collaboration.
CKMfitter Group.
UTfit Collaboration.

The full (dotted) lines correspond to the 68% (95%) C.L. regions. The star indicates the present world average.

>
>

15 years of $( \bar{\rho},~\bar{\eta} )$ predictions

Changed:

<
<

Evolution from 1988 to 2003 of the allowed region in the $(\bar{\rho},~\bar{\eta} )$ plane (contours at 68% and 95% probability are indicated by continuous black curves).

>
>

Evolution from 1988 to 2003 of the allowed region in the $(\bar{\rho},~\bar{\eta} )$ plane (contours at 68% and 95% probability are indicated by continuous black curves).

Revision 5

05 Apr 2010 - Main.VincenzoVagnoni

Line: 1 to 1

Added:

>
>

History of $\sin 2\beta$ predictions

Revision 4

04 Apr 2010 - Main.AdminUser

Line: 1 to 1
Changed:
< <
> >
	History of $\sin 2\beta$ predictions

Revision 3

04 Apr 2010 - Main.VincenzoVagnoni

-<
<
->
>
->
>
    History of  predictions
-<
<
->
>
     [EPS format]          [JPG format]
-<
<
->
>
 From left to right, they correspond to the following papers:
-<
<
->
>
 dRLMPPPPS90 (de Rujula, Lusignoli, Masetti, Pich, Petrarca, Prades, Pugliese, Steger), LHC Workshop Proc., Vol. II, CERN 90-10, ECFA 90-133, DEC. 1990.
-<
<
+DDGN90 (Dib, Dunietz, Gilman, Nir), Phys. ReV?. D41 (1990) 1522.
->
>
+DDGN90 (Dib, Dunietz, Gilman, Nir), Phys. Rev. D41 (1990) 1522.
 LMMR92 (Lusignoli, Martinelli, Maiani, Reina), Nucl. Phys. B369 (1992) 139.
 
AL94 (Ali, London), hep-ph/9405283.
 
CFMRS95 (Ciuchini, Franco, Martinelli, Reina, Silvestrini), Z. Phys C68 (1995) 239.
-<
<
+BBL96 (Buchalla, Buras, Lautenbacher), ReV?. Mod. Phys. 68(1996), 1125.
->
>
+BBL96 (Buchalla, Buras, Lautenbacher), Rev. Mod. Phys. 68(1996), 1125.
 AL96 (Ali, London), Nuovo Cimento 109A (1996) 957.
 
PPRS97 (Paganini, Parodi, Roudeau, Stocchi), Physica Scripta Vol. 58 (1998) 556-559.
 
BF97 (Buras, Fleischer), Adv. Ser. Direct. HEP 15 (1998) 65.
 B.et.al.00 (Bargiotti et al.), La Riv. del Nuovo Cimento Vol. 23 N3 (2000) 1.
 
HLLL00 (Hoecker, Laplace, Lacker, LeDiberder), Eur. Phys. J C21 (2001) 225.
 
and the latest value from this UTfit paper.
-<
<
->
>
 The dotted lines correspond to the 95% C.L. regions (the only information given in those papers). The larger bands (from year '99) correspond to values
of  from direct measurements.
-<
<
    History of  predictions
-<
<
->
>
-<
<
->
>
     [EPS format]          [JPG format]
     [EPS format]          [JPG format]
-<
<
->
>
 From left to right, they correspond to the following papers:
-<
<
->
>
 AL94 (Ali, London), hep-ph/9405283.
-<
<
+BBL95 (Buchalla, Buras, Lautenbacher), ReV?. Mod. Phys. 68(1996), 1125.
->
>
+BBL95 (Buchalla, Buras, Lautenbacher), Rev. Mod. Phys. 68(1996), 1125.
 AL96 (Ali, London), Nuovo Cimento 109A (1996) 957.
 
PPRS97 (Paganini, Parodi, Roudeau, Stocchi), Physica Scripta Vol. 58 (1998) 556-559.
 
BF97 (Buras, Fleischer), Adv. Ser. Direct. HEP 15 (1998) 65.
 HLLL00 (Hoecker, Laplace, Lacker, LeDiberder?), Eur. Phys. J C21 (2001) 225.
 
M01 (Mele), hep-ph/0103040.
 
UTfit Collaboration.
-<
<
+CKMfitter.
->
>
+CKMfitter Group.
 UTfit Collaboration.
-<
<
->
>
 The full (dotted) lines correspond to the 68% (95%) C.L. regions. The star indicates the present world average.
->
>

Revision 2

02 Apr 2010 - Main.VincenzoVagnoni

Line: 1 to 1

Changed:

<
<

Page under construction

>
>

History of $\sin 2\beta$ predictions

[EPS format] [JPG format] From left to right, they correspond to the following papers:

dRLMPPPPS90 (de Rujula, Lusignoli, Masetti, Pich, Petrarca, Prades, Pugliese, Steger), LHC Workshop Proc., Vol. II, CERN 90-10, ECFA 90-133, DEC. 1990.
DDGN90 (Dib, Dunietz, Gilman, Nir), Phys. ReV?. D41 (1990) 1522.
LMMR92 (Lusignoli, Martinelli, Maiani, Reina), Nucl. Phys. B369 (1992) 139.
AL94 (Ali, London), hep-ph/9405283.
CFMRS95 (Ciuchini, Franco, Martinelli, Reina, Silvestrini), Z. Phys C68 (1995) 239.
BBL96 (Buchalla, Buras, Lautenbacher), ReV?. Mod. Phys. 68(1996), 1125.
AL96 (Ali, London), Nuovo Cimento 109A (1996) 957.
PPRS97 (Paganini, Parodi, Roudeau, Stocchi), Physica Scripta Vol. 58 (1998) 556-559.
BF97 (Buras, Fleischer), Adv. Ser. Direct. HEP 15 (1998) 65.
BPS98 (Parodi, Roudeau, Stocchi), Il Nuovo Cimento 112A (1999) 883.
PS98 (Schune, Plaszczynski), hep-ph/9911280.
AL99 (Ali, London) Eur. Phys. J. C9 (1999) 687.
CFGLM99 (Ciuchini, Franco, Giusti, Lubicz, Martinelli), Nucl.Phys. B573 (2000) 201.
CPRS99 (Caravaglios, Parodi, Roudeau, Stocchi), hep-ph/0002171.
M99 (Mele), Phys. Rev. D59 (1999) 113011.
CDFLMPRS00 (Ciuchini, D'Agostini, Franco, Lubicz, Martinelli, Parodi, Roudeau, Stocchi), JHEP 0107 (2001) 013.
B.et.al.00 (Bargiotti et al.), La Riv. del Nuovo Cimento Vol. 23 N3 (2000) 1.
HLLL00 (Hoecker, Laplace, Lacker, LeDiberder), Eur. Phys. J C21 (2001) 225.
and the latest value from this UTfit paper.

The dotted lines correspond to the 95% C.L. regions (the only information given in those papers). The larger bands (from year '99) correspond to values of $\sin 2\beta$ from direct measurements.

History of $\Delta m_s$ predictions

[EPS format] [JPG format] From left to right, they correspond to the following papers:

AL94 (Ali, London), hep-ph/9405283.
BBL95 (Buchalla, Buras, Lautenbacher), ReV?. Mod. Phys. 68(1996), 1125.
AL96 (Ali, London), Nuovo Cimento 109A (1996) 957.
PPRS97 (Paganini, Parodi, Roudeau, Stocchi), Physica Scripta Vol. 58 (1998) 556-559.
BF97 (Buras, Fleischer), Adv. Ser. Direct. HEP 15 (1998) 65.
BPS98 (Parodi, Roudeau, Stocchi), Il Nuovo Cimento 112A (1999) 883.
AL00 (Ali, London) Eur. Phys. J. C9 (1999) 687.
CDFLMPRS00 (Ciuchini, D'Agostini, Franco, Lubicz, Martinelli, Parodi, Roudeau, Stocchi), JHEP 0107 (2001) 013.
B.et.al.00 (Bargiotti et al.), La Riv. del Nuovo Cimento Vol. 23 N3 (2000) 1.
HLLL00 (Hoecker, Laplace, Lacker, LeDiberder?), Eur. Phys. J C21 (2001) 225.
M01 (Mele), hep-ph/0103040.
UTfit Collaboration.
CKMfitter.
UTfit Collaboration.

The full (dotted) lines correspond to the 68% (95%) C.L. regions. The star indicates the present world average.

15 years of $( \bar{\rho},~\bar{\eta} )$ predictions

Evolution from 1988 to 2003 of the allowed region in the $(\bar{\rho},~\bar{\eta} )$ plane (contours at 68% and 95% probability are indicated by continuous black curves).

Difference: EvolutionPlots (1 vs. 8)

History of predictions

History of predictions

15 years of predictions

History of predictions

History of predictions

15 years of predictions

History of predictions

History of predictions

History of predictions

15 years of predictions

History of predictions

History of predictions

History of predictions

History of predictions

Page under construction

History of predictions

History of predictions

15 years of predictions

History of $\sin 2\beta$ predictions

History of $\Delta m_s$ predictions

15 years of $( \bar{\rho},~\bar{\eta} )$ predictions

History of $\sin 2\beta$ predictions

History of $\Delta m_s$ predictions

15 years of $( \bar{\rho},~\bar{\eta} )$ predictions

History of $\sin 2\beta$ predictions

History of $\sin 2\beta$ predictions

History of $\Delta m_s$ predictions

15 years of $( \bar{\rho},~\bar{\eta} )$ predictions

History of $\sin 2\beta$ predictions

History of $\sin 2\beta$ predictions

History of $\sin 2\beta$ predictions

History of $\Delta m_s$ predictions

History of $\sin 2\beta$ predictions

History of $\Delta m_s$ predictions

15 years of $( \bar{\rho},~\bar{\eta} )$ predictions