-
Notifications
You must be signed in to change notification settings - Fork 0
/
research.html
102 lines (60 loc) · 3.62 KB
/
research.html
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
97
98
99
100
101
102
<!DOCTYPE html>
<html>
<head>
<title> Research </title>
<link href="styles/style_general.css", type="text/css" rel="stylesheet" />
<link href="styles/style_research.css", type="text/css" rel="stylesheet" />
</head>
<body class="body" style="background-color:rgba(40,40,38,255);">
<div class="navbar">
<ul class="links">
<li> <a href="index.html"> Home </a></li>
<li> <a href="about.html"> Bio </a></li>
<li> <a class="active" href="research.html"> Research </a></li>
<li> <a href="papers.html"> Papers </a></li>
<li> <a href="cv.html"> CV </a></li>
<li> <a href="contact.html"> Contact </a></li>
</ul>
</div>
<div class="content">
<div class=info>
<div class="Research-interest">
<div style="font-family: Times, Arial, Helvetica;" class="current">
<p style="color:rgb(80, 200, 120);font-size: 2.1rem;opacity:0.9"> Current research </p>
My current work is centered on developing and testing analysis methods to apply the
pulse profile modeling technique to thermonuclear burst oscillation sources. In this endeavor, I predominantly use the open-source <a style="" href="https://github.com/xpsi-group/xpsi" target="_blank"> <em>X-PSI </em> </a>
package, where I contribute as both an advanced user and developer.
</div>
<div class="title">
<p style="margin-bottom: 0%;font-family: Times, Arial, Helvetica;color:rgb(80, 200, 120);font-size: 2.1rem;opacity:0.9">Research interests </p>
</div>
<div class="container">
<div class="container1">
<ul>
<li><span style="color: rgba(0,154,150,255); font-weight: bold; opacity:0.9"> High-energy astrophysics: </span>
neutron stars, neutron stars’ atmosphere, type-I X-ray bursts, burst oscillations </li>
<br>
<li><span style="color: rgba(0,154,150,255); font-weight: bold; opacity:0.9" > Computational (astro-) physics: </span>machine learning, high-performance computing & parallelization, Bayesian inference, nested sampling, Monte Carlo methods</li>
</ul>
</div>
<div class="container2">
<ul>
<li><span style="color: rgba(0,154,150,255);; font-weight: bold; opacity:0.9"> Nuclear physics:</span> equation of state of cold ultra-dense neutron matter</li>
<li><span style="color: rgba(0,154,150,255);; font-weight: bold; opacity:0.9"> High energy physics:</span> neutrino phenomenology and theory, beyond the standard model phenomenology </li>
</ul>
</div>
</div>
<div style="font-family: Times, Arial, Helvetica;" class="current">
<p style="color:rgb(80, 200, 120);font-size: 2.1rem;opacity:0.9"> Senior collaborators </p>
<a style="" href="https://www.uva.nl/en/profile/w/a/a.l.watts/a.l.watts.html#" target="_blank"> Anna L. Watts </a>(supervisor, UvA),
<a style="" href="https://www.uva.nl/en/profile/s/a/t.h.j.salmi/t.h.j.salmi.html" target="_blank"> Tuomo Salmi </a>(UvA),
<a style="" href="https://www.uva.nl/en/profile/v/i/s.v.vinciguerra/s.v.vinciguerra.html" target="_blank"> Serena Vinciguerra </a>(UvA),
<a style="" href="https://www.astro.columbia.edu/content/slavko-bogdanov" target="_blank"> Slavko Bogdanov </a>(Columbia),
<a style="" href="https://peterdenton.github.io/" target="_blank"> Peter B. Denton </a>(BNL),
<a style="" href="https://fit.uni-tuebingen.de/InternPerson/Details?id=7588" target="_blank"> Valery Suleymanov </a>(FIT).
</div>
</div>
</div>
</div>
</body>
</html>