Thursday, October 25, 2007

Beamline 10-2 Schedule (Nov 14 - Nov 20)

Beamline schedule (11/14/07 - 11/20/07)
Beamline 10-2 # 1-650-926-5102

11/14 (Wednesday)
8:30 am - 6:00 pm Bud / Jacob (setup)
5:00 pm - 1:00 am Bud
12:30 am - 9:00 am Justin

11/15 (Thursday)
8:30 am - 6:00 pm Bud / Carley / Anna
5:00 pm - 1:00 am Lisa
12:30 am - 9:00 am Justin

11/16 (Friday)
8:30 am - 6:00 pm Bud / Robert
5:00 pm - 1:00 am Jacob / John
12:30 am - 9:00 am Justin

11/17 (Saturday)
8:30 am - 6:00 pm
Lisa
5:00 pm - 1:00 am Justin
12:30 am - 9:00 am Jacob

11/18 (Sunday)
8:30 am - 6:00 pm Bud / John / Robert
5:00 pm - 1:00 am Justin
12:30 am - 9:00 am Jacob

11/19 (Monday)
8:30 am - 6:00 pm Bud
5:00 pm - 1:00 am Bud
12:30 am - 9:00 am Justin

11/20 (Tuesday)
8:30 am - 7:00 pm Bud / Justin (Breakdown)


Saturday, July 21, 2007

To my "compatriots"---an email to some common questions

My friends,

I am glad to receive emails regarding some application questions.

I have got some similar emails before, and I guess I will keep receiving them for the coming years. Therefore, I decide to publish my "answers" to those questions on the website, though they are only my narrow thoughts.

First, I am happy to choose UC Santa Cruz to continue my exploration on Physics, it's really a good small town for some one who loves ocean and forest. Plus, people are nice and warm-hearted here(most of the time), they won't lose patience to listen to my poor English.

Next, it's not too far to the Chinese civilization. 45 minutes driving distance to the nearest Chinese supermarkets, because it's close to the "Silicon Valley". The Asians' population at UCSC was said the lowest among UC system, but still very high, because it's CA.

In the Physics/Astronomy department at UCSC, there are some Chinese(7?), some are graduates while others are post-doc. The Physics Department recruits 10-15 graduate students each year. Depending on the bugdet, it will recruit 1-2 international students every year. I don't think we have any students without funding here. Normally, the first year students do TA, then depending on their choice, they may do RA or TA for the future years. I think it's a good practice to be a TA, because I can practice my English muscles.

In the Physics Department, we have several directions: High Energy and Cosmology, Experimental and Theoretical Condensed Matter. I am a condensed matter guy. I feel that every year, the population of new grads who are in favor of those research directions changes a lot. Therefore, I really can't say which direction has the best chance. I choose experimental condensed matter that year, just because I like it. If you like experimental condensed matter, we have several groups: one is doing neutron scattering, one is doing EXAFS, one is dong ARPES(these groups don't do experiments at UCSC, two of them do experiments at SSRL or LBNL, one at Argone or Los Almos, they do data analysis at school.); the other two labs are doing something like materials. If you get here, you can do one year rotation among any labs you are interested in.

Any way, if let me choose this year, I will still choose condensed matter.

If you have more questions, just send me a email.

By the way, I guess you just send emails to those whose names look like Chinese, however, some of them are domestic students, not international students, so they really know nothing about your questions.
Good luck!

So if you have further questions, I am happy to add more words on my website.

Tuesday, June 12, 2007

Beamline 10-2 Schedule (June 18 - June 25)

Mon (6/18)
Bud / Jesse (setup 10am - 5pm)
Jacob (5pm - 1am)
Justin (1am - 9am)

Tue (6/19)
Bud (9am - 6pm)
Lisa (5pm - 1am)
Justin (1am - 9am)

Wed (6/20)
Bud (9am - 6pm)
Jesse (5pm - 1am)
Lisa (1am - 9am)

Thur (6/21)
Bud / Nalini / Dave (9am - 6pm)
Jacob (5pm - 1am)
Jesse (1am - 9am)

Fri (6/22)
Justin (9am - 6pm)
Nalini (5pm - 1am)
Jesse (1am - 9am)

Sat (6/23)
Bud (9am - 6pm)
Jacob (5pm - 1am)
Nalini (1am - 9am)

Sun (6/24)
Dave / Justin (9am - 6pm)
Lisa / Ingrid (5pm - 1am)
Nalini (1am - 9am)

Mon (6/25)
Nalini / Lisa / Justin (Breakdown @ 6 am)

Wednesday, May 09, 2007

Beamline 10-2 Schedule (May 16 - 21)

Wed (5/16)
Bud / Justin (setup 10am - 5pm)
Bud / Jacob (5pm - 1am)
Lisa (1am - 9am)

Thur (5/17)
Geza (9am - 5:00pm)
Bud(3pm) / Jesse (5pm - 1am)
Justin (1am - 9am)

Fri (5/18)
Bud (9am - 5pm)
Geza (5pm - 1am)
Justin (1am - 9am)

Sat (5/19)
Lisa (9am - 5pm)
Jacob / Justin (5pm - 1:00am)
Jesse (1am - 9am)

Sun (5/20)
Bud (9am - 5pm)
Lisa (5pm - 1:00am)
Jesse (1am - 9am)

Mon (5/21)
Bud / Justin (Breakdown 6 am)

Saturday, March 03, 2007

Adding new 22% data





We can see the difference between the new mag31-22% data and the old 22% data. The step height of the new one is a little smaller that the old one. Which indicates that the new one is more like an "insulator" at low T.
The result is consistent with the change in the resistivity of the new 22% sample measured by J. J. Neumeier.

Thursday, February 22, 2007

Little Dog

LCMO data (x = 0.16-0.22)



Data points for LCMO (x = 0.16 - 0.22)

16% 18% 20% 22%
3 3 3 3
20 20 20 20
40 40 40 40
60 60 60 60
80 70 70 80
100 100 100 100
120 120 120 105
135 135 135 120
140 140 140 135
150 150 150 140
155 155 155 150
160 160 160 155
170 170 170 160
175 175 180 170
180 180 185 175
185 185 190 180
195 190 195 185
200 195 200 190
210 200 210 195
220 210 225 195
250 225 250 200
260 250 270 210
270 270 275 220
300 275 308 250
308 308 320 260
340 320 348 270
348 348 398 300
398 398 448 303
448 448 498 345
498 498 555 376
555 555
406



435



465



495



524



555

Wednesday, January 24, 2007

Preliminary results by ananlyzing LCMO (16%-22%)















This is the Sigma^2 vs T for different samples with doping level x = 16%,18%,20%,22%.

A sharp increase in Sigma^2 (Sigma is the width of the Mn-O pair distribution function "PDF")near Tc.

The magnitude of the step decreases rapidly with decreasing x.

The value of Sigma^2 at low T is close to the value for zero-point motion for x = 22%, but increases substantially for lower x, which indicates that in the magnetized state there is either a large Jahn-Teller distortions or a static distortion which remains at low T.

The end compound LaMnO3 has a large J-T distortion, so we think it's caused by J-T distortion.














Also the magnetization at low T is small for lower x, indicating that not all of the sample is ferromagnetic, regions of antiferromagnetism may remain.